Real-time dynamics in the 1+1 D abelian Higgs model with fermions

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你想要和哪位名人一起吃晚饭英语口语作文

你想要和哪位名人一起吃晚饭英语口语作文

你想要和哪位名人一起吃晚饭英语口语作文全文共6篇示例,供读者参考篇1Who Would I Want to Have Dinner With?If I could have dinner with any famous person in the world, I would pick Neil Armstrong. He was the first person ever to walk on the moon! How awesome is that? I've been really interested in space and astronauts ever since we learned about the moon landing in science class last year.I have so many questions I would love to ask Mr. Armstrong about his time in space. What was it like taking that first step onto the lunar surface? Did he feel nervous or scared at all? The moon's gravity is much lower than Earth's, so did he feel lighter or was it hard to walk? I heard the moon dust was really thick and stuck to everything - was that true? What did he think when he first looked up at the Earth from the moon? It must have been an incredible view.I'd ask him to tell me all the details about blasting off into space aboard the huge Saturn V rocket. I saw videos of a launch in class and the flames and smoke billowing out looked unreal. Ican't imagine how loud it must have been or how much shaking there was during liftoff with all those powerful engines firing. Did it make his stomach do flips? I get a little queasy sometimes on roller coasters!Once they made it to the moon, I want to know what it was like living and working inside the little lunar module for all those days. The module couldn't have been much bigger than a camper, yet Mr. Armstrong and Mr. Aldrin were stuck inside for over 21 hours before walking on the moon. That seems so cramped! Did they get cabinfever? How did they go to the bathroom? I've heard astronauts have to use diapers on spaceflights - is that true or just a rumor?So many kids dream of becoming an astronaut when they grow up. I would pick his brain to find out the best way to make that dream come true. Like, what were his favorite subjects in school? Did he struggle with any particular topics? What first sparked his interest in space and exploring? What advice would he give me and other kids who hope to walk on the moon themselves one day? I'd write down every word so I wouldn't forget a thing!After grilling him with a million questions about space, I'd be really curious to learn more about him as a regular person too.Did he have hobbies and interests outside of his astronaut work? What kind of music and TV shows did he enjoy? What were some of his most prized possessions? If he could pick his absolute favorite meal, what would it be? I'd make sure to request that meal from my parents so I could serve it to him at our dinner. I bet he hasn't had a real home-cooked meal in a while!After he told me everything there was to know about being an astronaut and space travel, I'd ask Mr. Armstrong about other parts of his life too. Like what the biggest challenges or struggles he had to overcome in his life and career were. And what he is most proud of, besides the moonwalk. Those topics would probably lead to some good life lessons and inspiration that I could learn from.Then, once Mr. Armstrong and I were well into our moonwalk meal, I'd switch to some silly, fun questions to keep the conversation light. Like if aliens did exist, what would he want to say to them? Or which movies about space does he think got it totally wrong? Fun questions like that would be a great way to end our time together on a high note.After dinner, I'd obviously need to get his autograph and take a photo with him to prove to my classmates that I really did have dinner with Neil Armstrong, the first human on the moon!Maybe if I'm lucky he'd even let me try on his famous spacesuit for a picture. Can you imagine how awesome that would be?Meeting and talking to Neil Armstrong would be a dream come true. His moonwalk is one of the most incredible things any human being has ever done. Having dinner with the first man to walk on the moon would easily be the coolest experience of my whole life so far. Just thinking about being able to ask him all my million questions gets me so excited! I'd make sure to soak in and remember every second so I could tell everyone about it for years to come.篇2Who Would I Want to Have Dinner With?If I could have dinner with any famous person in the whole world, I would pick Michael Jordan! He is my biggest hero and the person I look up to the most. Let me tell you all the reasons why.First of all, Michael Jordan is one of the greatest basketball players ever. He led the Chicago Bulls to six NBA championship wins in the 1990s. Michael could jump really high and dunk the ball in amazing ways. He had a cool nickname too - "Air Jordan" because he seemed to fly through the air when he played. I lovewatching videos of his best plays and moves on the court. He was so talented and worked incredibly hard to be the best.But it's not just his basketball skills that make me admire Michael Jordan so much. He also seems like a really good person off the court too. Despite becoming a huge celebrity and making tons of money, he has stayed humble and kind. Michael has raised millions of dollars for charity through his Jordan brand and camps for kids. He overcame obstacles like being cut from his high school basketball team early on and used it as motivation. His determination and perseverance are so inspiring.If Michael Jordan came over for dinner, I would ask him a million questions! I would want to know what it felt like to hit the winning shot in an NBA Finals game. Did he ever get nervous or scared before big games? What were his hobbies and interests outside of basketball? I would ask for all his best tips and advice for working hard, setting goals, and never giving up. Maybe he could even teach me some of his signature basketball moves in the driveway after we ate!I can picture it so clearly - Michael Jordan sitting at my family's dinner table, my mom's delicious spaghetti on his plate. I would hang on his every word as he told stories from his playing days with the Bulls. He could meet my dog Rufus and we couldshow him our basketball hoop in the backyard. After dinner, we could play some games of P-I-G or just shoot around for fun. Michael Jordan has always been my favorite athlete, but if I got to know him in person too, he could become my heroic friend as well.It would be a dream come true to have dinner with the legendary Michael Jordan. His talents, mindset, and personality make him someone I hugely look up to. I would cherish every moment and bit of wisdom from an amazing athlete and role model like him. Just thinking about it gives me goosebumps! Even though I'm just a kid who loves the game of basketball, I have big dreams and goals inspired by Michael Jordan's excellence and spirit. With his guidance and spending time together over a meal, who knows what heights I could reach? The sky is the limit when you dine with HisAirNess himself!篇3Who I Would Want to Have Dinner WithIf I could have dinner with any famous person in the whole wide world, I would choose to have dinner with Queen Elizabeth II. She was the Queen of England for a really really long time - over 70 years! I think it would be so cool to meet a real queen.I have learned all about Queen Elizabeth II in my history and English classes at school. She became queen in 1952 when she was just 25 years old after her father King George VI passed away. Can you imagine being made the queen of an entire country at 25? I'll be 25 in about 19 more years and I can't even imagine being in charge of running a whole country at that age! Queen Elizabeth II must have been very brave and responsible.Queen Elizabeth II had such an exciting and glamorous life. She lived in huge fancy palaces like Buckingham Palace and went to lots of special events and parties. But she also worked very hard her whole life and took her job as queen extremely seriously. She had to make lots of important decisions and go on many trips around the world to meet with leaders of other countries. I don't know if I would want all of that responsibility!One of the things I admire most about Queen Elizabeth II is how dedicated she was to her country and people. She always put Great Britain first, before herself. My parents are always telling me how important it is to think about others instead of being selfish. Queen Elizabeth II was definitely not selfish - she devoted her entire life to public service until the very end when she passed away in 2022 at the incredible age of 96.I have so many questions I would want to ask Queen Elizabeth II if I could have dinner with her. I would ask her what it was like to be crowned the queen as a young woman. I can't even imagine how nervous she must have felt! I would ask her if she ever got tired of all the rules and traditions she had to follow as the queen. It seems like it would be hard to always have to act so properly in public. I know I wouldn't like that part!I would also ask Queen Elizabeth II about the most fun or exciting parts of being the queen. What was her favorite royal event or party she got to attend? Did she like traveling all around the world and if so, what was her favorite country she visited?I've hardly ever traveled outside of my own state, so I'm very curious to learn what traveling is like from someone who went to so many amazing places.Another thing I would definitely ask Queen Elizabeth II about is her family. She had four children, including her oldest son Charles who became King Charles III when she passed away. I would want to know what it was like raising children while also being the monarch. Did her kids have to follow a bunch of strict rules too or did they get to act like normal kids sometimes? I can't even imagine how difficult it would be to try to be both a good parent and a good queen at the same time!Queen Elizabeth II had such an extraordinary life and I have so much respect and admiration for how gracefully and honorably she conducted herself on the world stage until the very end. She was an icon of strength, dignity and duty. I may only be 9 years old, but I know that having the chance to meet Queen Elizabeth II and hear her stories over a nice dinner would be a remarkable and unforgettable experience. She was a true model of leadership, courage and faith that I hope I can be inspired by as I grow up. The world could definitely use more people as noble as Her Majesty the Queen.That's why Queen Elizabeth II is the famous person I would want to have dinner with more than anyone else. She seemed like such a classy lady with amazing experiences to share. It would be a night I would never, ever forget - a young kid like me getting to share a meal fit for a queen! Maybe she could even give me some lessons on proper etiquette and manners. I may need all the help I can get to learn not to chew with my mouth open or talk with my mouth full! Having dinner with the Queen of England would certainly be an incredible honor I could tell my grandkids about someday. So if you're reading this, your Majesty, please save me a seat at your royal table!篇4Who Would I Want to Have Dinner With?If I could have dinner with any famous person, I would pick Michael Jackson! He was the King of Pop and made some of the best music ever. I love dancing around my room and singing along to his songs like "Billie Jean", "Beat It", and "Thriller". His dance moves were just so cool and smooth. He could spin and kick and pop like nobody else. I try to copy his moves but I'm not nearly as good as he was.Michael Jackson was a real-life Peter Pan too. He had his own private theme park called Neverland Ranch with a roller coaster, Ferris wheel, and even a zoo! How awesome would it be to go on all those rides with him after we finished our dinner? Maybe we could have a sleepover in the castle there too. We could stay up late watching movies, eating popcorn, and telling spooky stories. I bet he would do such great impersonations of the characters' voices!For our dinner, I think we should have his favorite foods. I read that he really liked fried chicken, mashed potatoes, and baked beans. My mom makes the best fried chicken so maybe she could cook for us. Michael could teach me how to do the anti-gravity lean move while we ate. Although for dessert, we'ddefinitely need to have a huge ice cream sundae! Chocolate sauce, sprinkles, whipped cream, cherries, the works!I have so many questions I would ask him over our dinner too. Like how did he come up with the ideas for his music videos that were like short movies? The ones for "Thriller" and "Smooth Criminal" were so creative and spooky. I loved the dance scene at the end of "Thriller" with all the zombie dancers. I want to know how long it took to learn those dances and film it all.I'd also ask him about the first song he ever wrote and what inspired it. What was it like being a child star? Did he have a regular childhood at all or was he always working and practicing? It must have been so tough having photographers and fans following him everywhere, even as a little kid. I wouldn't want that, I like my privacy! Although maybe if I was as talented as him, I wouldn't mind.Another thing I'd really want to know is how he came up with the anti-gravity lean move and if it was hard to pull off. He would lean way forward but somehow still stay upright and vertical. It didn't look physically possible! Was there a special trick to it or was he just incredibly well-balanced? I've tried copying that one and I can't do it at all without falling over. I need him to teach me.And of course, I'd ask him about all the different outfits, accessories, and sweet dance moves he did. Why did he like wearing just one glove sometimes? What was the deal with the sparkly socks and penny loafers? Those were definitely a unique look! And his signature spin move, the moonwalk, and "Beat It" choreography - I'd need him to break it all down for mestep-by-step.We could try on some of his iconic looks together after dinner too. I'd let Michael do my hair and makeup however he wanted. Maybe he could even get me a matching red jacket to his "Thriller" one! Then we could reenact the "Beat It" music video together in the backyard. Just us two testing out all the punches, spins, and kicks. That would be so epic.Michael Jackson was one of the greatest performers and entertainers ever. It's hard to imagine anyone else I'd rather have dinner with. I could talk to him all night long about his incredible life, music, and dance skills. It would be a night I'd never, ever forget. Maybe if I'm really good, he could even let me stay at Neverland and we could be best friends forever!篇5If I Could Have Dinner with Any Famous PersonDo you ever wonder what it would be like to meet someone famous? I think about it all the time! There are so many incredible people out there who have done amazing things. If I could have dinner with any famous person, I would choose Neil Armstrong, the first person to walk on the moon!Neil Armstrong is my biggest hero. I've learned all about him in school, and I've read books and watched movies about his incredible journey to the moon. Can you imagine being the first human ever to set foot on another world? That must have been the most exciting and terrifying experience ever!I would love to have dinner with Neil Armstrong so I could ask him all sorts of questions about his trip to the moon. What was it like to blast off in the giant Saturn V rocket? Did he get scared or nervous at all during the mission? How did it feel to take those first steps on the lunar surface? I've seen the famous footage of him bouncing around in the moon's lower gravity, but I'd love to hear him describe it in his own words.I'd ask him what it was like to look back at the Earth from so far away. The photos of our beautiful blue planet hanging in the blackness of space are some of the most amazing images I've ever seen. Did it make him feel small and insignificant, or did itfill him with a sense of wonder and appreciation for our incredible home?And after he walked on the moon, what was it like to lift off from the lunar surface and rendezvous with the command module piloted by Michael Collins? That must have been such a tense and difficult maneuver. I'd ask him to walk me through every step of that process.Neil Armstrong spent a total of 21 hours on the lunar surface during the Apollo 11 mission. I can't even begin to imagine how mind-blowing that experience must have been. To be the first person to witness the majesty of the moon up close... There's just no way to describe how incredible that must have felt.And I'd be really curious to learn about his life after NASA as well. How did he adjust to being a regular person again after achieving such an incredible feat? Did people treat him differently or act weird around him? What did he end up doing for work after leaving the astronaut corps?Maybe he could share some wisdom about setting big goals and working hard to achieve your dreams. As a little kid, becoming an astronaut and walking on the moon must have seemed like an impossible long shot. But Neil Armstrong nevergave up on his dream, and through dedication and perseverance, he accomplished something that will be remembered forever.I have so many dreams of my own – becoming a scientist or an explorer, traveling to other planets, making an important discovery that changes the world. Hearing Neil Armstrong's stories and getting his advice would be so inspiring. He could tell me what it really takes to transform your wildest dreams into reality.Although he's an American hero who achieved one of the greatest feats in human history, I'll bet Neil Armstrong is probably just a regular, down-to-earth guy at heart. He was an engineer and a pilot before becoming an astronaut, and I imagine he maintains that same humble, hard-working spirit even after all his accomplishments.I'd love to ask him how he stayed so calm and focused under immense pressure. I get flustered really easily sometimes, like when I have to give a presentation in front of my whole class. But Neil Armstrong had the weight of the entire world on his shoulders during that first moon landing, and he didn't let it faze him one bit! What's his secret for keeping your cool in stressful situations?Spending an evening with Neil Armstrong would be a dream come true. I'm sure I'd be a little starstruck at first, but I'd do my best to stay composed and make the most of our time together. This could be a once-in-a-lifetime opportunity to gain wisdom and insight from one of the greatest explorers and adventurers who ever lived.And who knows, maybe by the end of the night, Neil Armstrong would be just as inspired by me as I am by him! I'd tell him all about my passion for science and my goals for the future. Maybe I could share some of my latest ideas about space exploration or pitch him some theories I've been working on. You never know – perhaps I could dazzle him with my intelligence and curiosity!Whether we spent the evening discussing the wonders of space, sharing stories from our lives, or chatting about our biggest dreams and ambitions, I know it would be a truly unforgettable experience. Getting to meet one of my biggest heroes and idols, the first man to walk on the moon, would be an incredible honor. I can only imagine how much I could learn from him and how inspired I would feel after our dinner together.So if I ever get the chance to have a meal with a famous person, you can bet I'll be putting Neil Armstrong at the top ofmy list. He's led a life of daring adventure and groundbreaking achievement. What could be cooler than breaking bread with the first human being to set foot on another celestial body? To me, that sounds like the most epic dinner date ever!篇6If I Could Have Dinner With Any Famous PersonHave you ever wondered what it would be like to sit down and have a real conversation with someone famous? I think about that a lot. There are so many incredible people throughout history who have done amazing things. If I could pick just one person to have dinner with, it would definitely be...Marie Curie!Marie Curie was a brilliant scientist who made some of the most important discoveries about radiation and radioactivity. She was the first woman to win a Nobel Prize, and get this - she actually won two Nobel Prizes during her lifetime! One was for Physics in 1903, and the other was for Chemistry in 1911. How awesome is that?I would love to have dinner with Marie Curie because I'm really curious about what motivated her and how she overcame all the obstacles in her way as a woman in science back in thosedays. It must have been so difficult with people not taking her seriously just because she was a woman. But she never gave up!I can picture us sitting at a little cafe in Paris, sipping hot chocolate, and I'd ask her "Miss Curie, what inspired you to dedicate your life to science?" I bet her answer would be fascinating. Maybe she'd tell me about her childhood in Poland and how her parents valued education. Or perhaps she'd describe her early days as a governess before she could enroll at the Sorbonne University in France.I have a million other questions I'd want to ask too. Like what it was like being one of the few female students at an elite university at that time? How did she balance her research work with being a wife and mother? What gave her the courage and determination to keep going when so many people doubted her just because of her gender?It would be incredible to hear straight from Marie Curie how she and her husband Pierre discovered the radioactive elements radium and polonium. I've read that they had to work in an old shed and separate the radioactive materials from tons of the mineral pitchblende through very dangerous processes. Imagine doing that revolutionary research in conditions like that!I'd be so excited to ask her about the Curie portable x-ray units that she helped develop during World War I. Those units saved so many lives by making it possible to easily x-ray soldiers and find bullets or shrapnel inside their bodies on the battlefields. Marie Curie was even directly involved in operating those x-ray units at the front lines, risking her own life from all the radiation exposure. What bravery!I have a feeling dinner with Marie Curie would be such an inspiring experience. Just being in the presence of someone who overcame incredible prejudices, worked with unwavering passion and purpose, and literally changed the world through her discoveries - it would be simply amazing. Her life story proves that with enough courage, brilliance, and perseverance, any young person really can grow up to accomplish extraordinary things.After our cafe dinner, maybe we could go for a walk along the riverbank and Marie Curie could tell me more about her fascinating life and work. I'd try to soak in every word from this pioneer who opened so many new frontiers for women in science. Meeting her greatest living role model would definitely make that the best dinner ever for this kid who dreams of making the world a better place someday too.So if I could choose any famous person throughout history to share a meal with, there's no doubt it would be the incredible Madame Marie Curie. Getting life lessons and insights straight from someone of her genius and character would be an unforgettable experience that could inspire me for years to come.I can't think of any other person I admire more for their brilliance, resilience and world-changing accomplishments. Marie Curie is simply the top pick for my fantasy dinner guest!。

dAlembert

dAlembert

Jean Le Rond d'AlembertBorn: 17 Nov 1717 in Paris, FranceDied: 29 Oct 1783 in Paris, France法国数学家、力学家、哲学家。

他是一位贵妇人的私生子,出生后被遗弃,由一对玻璃匠夫妇抚养成人。

早年学习法律和医学,后转向自然科学。

1739年,他在巴黎科学院宣读第一篇论文,1741年当选为科学院院士,1754年称为法兰西学院院士,1772年担任学院终身秘书,还被选为多国科学院院士。

达朗贝尔在力学方面做出了杰出的贡献。

他在1743年发表了关于动力学的一部基础性著作《论动力学》,提出了动力学基本规律-达朗贝尔原理。

达朗贝尔的数学研究主要在微分方程、复变函数、级数理论和无穷小分析等方面。

1747年,他在研究弦振动问题的论文中给出了著名的弦振动方程及其通解。

他与欧拉、丹尼尔∙伯努利的工作共同奠定了数学物理方程的基础。

他在流体力学论文《关于流体阻力的新理论》中,首先应用了复变函数,并推导出表示解析函数实部和虚部关系的基本方程,为复变函数理论的建立做出了贡献。

在常微分方程理论中,他得到了常系数线性方程和一阶、二阶线性方程组的重要结果。

他首次给出了判别正项级数收敛的充分条件-达朗贝尔法则,还曾试图建立严格的极限理论。

他的主要数学著作编辑成了8卷集的《数学论文集》。

达朗贝尔是18世纪法国启蒙运动的领袖人物之一。

他和唯物主义哲学家狄德罗是朋友,他们共同编纂了《百科全书》(共35卷,1751-1780年出版)。

他在该书前言中提出百科全书要以统一的观点反映当代知识,追溯发展历史,研究各学科分支间的关系,并显示出它们如何融为一体。

他还为《百科全书》撰写了“微分”、“方程”、“动力学”、“几何学”、“维数”、“哲学原理”等重要条目。

在“维数”一文中,他首先把时间作为第4维空间提出。

达朗贝尔还致力于哲学研究,他主张理性和自然的权力,反对旧教条和旧制度,拥护社会改良。

An Introduction to Seismology, Earthquakes, and Earth Structure

An Introduction to Seismology, Earthquakes, and Earth Structure

3
Seismology and Earth Structure, 119
3.7.3 Multipathing,187 3.7.4 Scattering, 189 3.7.5 Intrinsic attenuation, 190 3.7.6 Quality factor, Q, 192 3.7.7 Spectral resonance peaks, 193 3.7.8 Physical dispersion due to anelasticity, 194 3.7.9 Physical models for anelasticity, 196 3.7.10 Q/row crustto inner core, 197 3.8 Composition of the mantle and the core, 198 3.8.1 Density within the earth, 199 3.8.2 Temperature in the earth, 203 3.8.3 Composition of the mantle, 204 3.8.4 Composition of D", 208 3.8.5 Composition of the core, 209 3.8.6 Seismology and planetary evolution, 210 Further reading, 212 Problems, 212
4
Earthquakes, 215
4.1 Introduction, 215 4.2 Focal mechanisms, 217 4.2.2 Fault geometry, 217 4.2.2 First motions, 219 4.2.3 Body wave radiation patterns, 220 4.2.4 Stereographic fault plane representation, 222 4.2.5 Analytical representation of fault geometry, 228 4.3 Waveform modeling, 229 4.3.2 Basic model, 229 4.3.2 Source time function, 230 4.3.3 Body wave modeling, 231 4.3.4 Surface wave focal mechanisms, 235 4.3.5 Once and future earthquakes, 239 4.4 Moment tensors, 239 4.4.2 Equivalent forces, 239 4.4.2 Single forces, 240 4.4.3 Force couples, 241 4.4.4 Double couples, 242 4.4.5 Earthquake moment tensors, 242 4.4.6 Isotropic and CLVD moment tensors, 245 4.4.7 Moment tensor inversion, 246 4.4.8 Interpretation of moment tensors, 249 4.5 Earthquake geodesy, 251 4.5.1 Measuring ground deformation, 251 4.5.2 Coseismic deformation, 254 4.5.3 Joint geodetic and seismological earthquake studies, 256 4.5.4 Interseismic deformation and the seismic cycle, 259 4.6 Source parameters, 263 4.6.2 Magnitudes and moment, 263 4.6.2 Source spectra and scaling laws, 266 4.6.3 Stress drop and earthquake energy, 269 4.7 Earthquake statistics, 274 4.7.2 Frequency-magnitude relations, 2 74

基于改进切线角实时算法的滑坡监测预警

基于改进切线角实时算法的滑坡监测预警

第 22卷第 11期2023年 11月Vol.22 No.11Nov.2023软件导刊Software Guide基于改进切线角实时算法的滑坡监测预警贾丁1,2,陈小红1,2,周永贵1,2(1.航天宏图信息技术股份有限公司,北京 100089;2.自然资源部地质灾害智能监测与风险预警工程技术创新中心,北京 100081)摘要:全球卫星导航系统(GNSS)在地质灾害监测预警领域应用广泛,由其位移—时间曲线计算得到的改进切线角是滑坡监测预警模型中的重要判据。

现有的改进切线角计算方法计算结果波动性大,匀速变形阶段速度选取随机性强,导致计算准确性和时效性较低。

鉴于此,实现了一种改进的切线角算法,采用拉格朗日插值微分的五点法可将计算准确度提升77.33%。

同时,通过匀速阶段判识方法和设置速度更新条件,实现了切线角的动态实时计算,为滑坡监测预警提供实时、动态判据,提高了滑坡监测预警实用性。

关键词:GNSS;切线角;位移—时间曲线;滑坡;监测预警DOI:10.11907/rjdk.231778开放科学(资源服务)标识码(OSID):中图分类号:TP399;P642.2 文献标识码:A文章编号:1672-7800(2023)011-0035-07Landslide Monitoring and Warning Based on Improved Tangent AngleReal-time AlgorithmJIA Ding1,2, CHEN Xiaohong1,2, ZHOU Yonggui1,2(1.PIESAT Information Technology Co., Ltd, Beijing 100089,China;2.Geological Disaster Intelligent Monitoring and Risk Early Warning Engineering Technology Innovation Center of the Ministry of Natural Resources,Beiijng 100081,China)Abstract:GNSS (Global Navigation Satellite System) is widely used in the field of geological disaster monitoring and warning. The improved tangent angle calculated from its displacement time curve is an important criterion in landslide monitoring and warning models. The existing im‑proved tangent angle calculation methods have high fluctuation in the calculation results, and the selection of velocity during the uniform defor‑mation stage has strong randomness, resulting in low calculation accuracy and timeliness. This article implements an improved tangent angle algorithm,which uses the five point method of Lagrange interpolation differentiation to improve computational accuracy,increasing by 77.33%. And through the uniform speed stage identification method and setting speed update conditions, the dynamic real-time calculation of tangent angle is achieved, providing real-time and dynamic criteria for landslide monitoring and warning, and improving the practicality of landslide monitoring and warning.Key Words:GNSS; tangent angle; displacement-time curve; landslide; monitoring and early warning0 引言我国地质灾害频发,滑坡作为我国最主要的地质灾害类型之一,严重威胁人民生命财产安全。

hbm t11000 测量系统 使用说明书

hbm t11000 测量系统 使用说明书

Introduction to HBM presentation Challenges in dynamic torque and force measurement with special regard to industrial demands for the dynamic measurement workshop held at BIPM, Paris, November 2012.by Dr.-Ing. André Schäfer, HBM, Darmstadt Germany, Collaborator in IND09 ProjectFor more than six decades we have served many branches of industry as a manufacturer of complete measuring chains from the sensor via data processing to software. The first products were amplifiers and inductive transducers. In 1955 the company started –as the first company in Europe - the production of strain gauges, marking the beginning of a big success story. Today reference transducers and precision instruments in static calibration for quantities such as force, torque and pressure are carried out with strain gauges, as this allows the smallest possible measurement uncertainty for the whole measuring chain. So it is no wonder that HBM was the first calibration laboratory in the German Calibration Service (DKD) in 1977.To cope with the new challenges we take part in several projects in the framework of EURAMET. This includes both the EMRP (European Metrology Research Programme) projects but recently also its successor, EMPIR (European Metrology Programme for Innovation and Research).What makes the EMRP project JRP IND09 Traceable Dynamic Measurements of Mechanical Quantities outstanding is its vision. Although static calibration is still the underlying reality today, the automotive industry especially is very interested in dynamic calibration research with a focus on mechanical quantities.One key issue is dynamic force and torque calibration and, in particular, considerations of varying uncertainty of measurement when using a force or a torque transducer for calibration or for a specific application. In the field of force transducers, this applies mainly for aerospace and materials testing (e.g., in material testing machines). In the field of torque, automotive and shipbuilding applications are of interest, so in-line torque measurement is required, i.e., measurement directly on the drive train of ships. Tightened regulations (e.g., for emission limits) require a substantial increase in accuracy of torque measurement. Eventually, both rotational speed measurement and power must be certified.We are well aware of the fact that the uncertainties of measurement that can be achieved with dynamic calibration will - for the time being or in principle even permanently –be markedly more significant than those already attainable with static measurements today. It is essential that expectations remain realistic but also reflect industry requirements, because what we offer is - compared to today's ignorance of these influences – is real progress and closer to the truth. Torque users in industry are primarily interested in what torque is acting on the test specimen, to what extent the measurement devices, electronics, and shaft train affect the actual loading, and how this has to be taken into account.For torque a key feature that has to be considered is that today torque transducers are mounted in a calibration machine in a non-rotating setup, while industrial users are interested in rotating conditions, so dynamic in the real application. Dynamic calibration is the logical successor of static calibration. However standards, regulations or even design rules for dedicated transducers have to be created. Thus the EMRP project helps to close the gap between the present and future demands of industry and what NMIs and suppliers can offer today.A great milestone in the project was the participation in the workshop on Challenges in Metrology for Dynamical Measurement that took place at the BIPM (Bureau International des Poids et Mesures) in November 2012. From the HBM presentation one could see that for torque and force measurement foil type strain gauge transducers are most accurate and with steel and titanium measuring body realisations one can also go up to very high force and torque values. HBM offers complete measuring chains. The workshop also addressed the difficulty that the dynamic behavior of the complete system in the application will differ much from that of the component delivered by HBM (transducer + digital acquisition systems).The main conclusion have been that measuring chain realisations at national level as well as reference transducers have to be as effective as possible and at industrial level first of all affordable. HBM pointed out that the dynamic behavior of the complete system in the application at the customer will differ greatly from that of the component delivered by HBM (the transducer). So the total system clearly has to be considered. Nevertheless the components clearly have to be understood and evaluated.We are proud to contribute to first guidelines on products and regulations for the traceability of dynamic measurements of mechanical quantities along with the final phase of EMRP JRP IND09 project. We hope that continue that contribution also to enhance our general reputation as a company driving future technology.。

Existence of Infinitely Many Solutions for a Quasilinear Elliptic Problem on Time Scales

Existence of Infinitely Many Solutions for a Quasilinear Elliptic Problem on Time Scales
Let f : T → R and t ∈ Tk (assume t is not left-scattered if t = sup T). We define f △(t) to be the number (provided it exists) such that given any ǫ > 0 there is a neighborhood U of t such that
arXiv:0705.3674v1 [math.AP] 24 May 2007
Existence of Infinitely Many Solutions for a Quasilinear Elliptic Problem on Time Scales
Moulay Rchid Sidi Ammi sidiammi@mat.ua.pt
2 Preliminary results on time scales
We begin by recalling some basic concepts of time scales. Then, we prove some preliminary results that will be needed in the sequel.
Delfim F. M. Torres delfim@mat.ua.pt
Department of Mathematics
University of Aveiro 3810-193 Aveiro, Portugal
Abstract
We study a boundary-value quasilinear elliptic problem on a generic time scale. Making use of the fixed-point index theory, sufficient conditions are given to obtain existence, multiplicity, and infinite solvability of positive solutions.

不对称约束多人非零和博弈的自适应评判控制

第40卷第9期2023年9月控制理论与应用Control Theory&ApplicationsV ol.40No.9Sep.2023不对称约束多人非零和博弈的自适应评判控制李梦花,王鼎,乔俊飞†(北京工业大学信息学部,北京100124;计算智能与智能系统北京市重点实验室,北京100124;智慧环保北京实验室,北京100124;北京人工智能研究院,北京100124)摘要:本文针对连续时间非线性系统的不对称约束多人非零和博弈问题,建立了一种基于神经网络的自适应评判控制方法.首先,本文提出了一种新颖的非二次型函数来处理不对称约束问题,并且推导出最优控制律和耦合Hamilton-Jacobi方程.值得注意的是,当系统状态为零时,最优控制策略是不为零的,这与以往不同.然后,通过构建单一评判网络来近似每个玩家的最优代价函数,从而获得相关的近似最优控制策略.同时,在评判学习期间发展了一种新的权值更新规则.此外,通过利用Lyapunov理论证明了评判网络权值近似误差和闭环系统状态的稳定性.最后,仿真结果验证了本文所提方法的有效性.关键词:神经网络;自适应评判控制;自适应动态规划;非线性系统;不对称约束;多人非零和博弈引用格式:李梦花,王鼎,乔俊飞.不对称约束多人非零和博弈的自适应评判控制.控制理论与应用,2023,40(9): 1562–1568DOI:10.7641/CTA.2022.20063Adaptive critic control for multi-player non-zero-sum games withasymmetric constraintsLI Meng-hua,WANG Ding,QIAO Jun-fei†(Faculty of Information Technology,Beijing University of Technology,Beijing100124,China;Beijing Key Laboratory of Computational Intelligence and Intelligent System,Beijing100124,China;Beijing Laboratory of Smart Environmental Protection,Beijing100124,China;Beijing Institute of Artificial Intelligence,Beijing100124,China)Abstract:In this paper,an adaptive critic control method based on the neural networks is established for multi-player non-zero-sum games with asymmetric constraints of continuous-time nonlinear systems.First,a novel nonquadratic func-tion is proposed to deal with asymmetric constraints,and then the optimal control laws and the coupled Hamilton-Jacobi equations are derived.It is worth noting that the optimal control strategies do not stay at zero when the system state is zero, which is different from the past.After that,only a critic network is constructed to approximate the optimal cost function for each player,so as to obtain the associated approximate optimal control strategies.Meanwhile,a new weight updating rule is developed during critic learning.In addition,the stability of the weight estimation errors of critic networks and the closed-loop system state is proved by utilizing the Lyapunov method.Finally,simulation results verify the effectiveness of the method proposed in this paper.Key words:neural networks;adaptive critic control;adaptive dynamic programming;nonlinear systems;asymmetric constraints;multi-player non-zero-sum gamesCitation:LI Menghua,WANG Ding,QIAO Junfei.Adaptive critic control for multi-player non-zero-sum games with asymmetric constraints.Control Theory&Applications,2023,40(9):1562–15681引言自适应动态规划(adaptive dynamic programming, ADP)方法由Werbos[1]首先提出,该方法结合了动态规划、神经网络和强化学习,其核心思想是利用函数近似结构来估计最优代价函数,从而获得被控系统的近似最优解.在ADP方法体系中,动态规划蕴含最优收稿日期:2022−01−21;录用日期:2022−11−10.†通信作者.E-mail:***************.cn.本文责任编委:王龙.科技创新2030–“新一代人工智能”重大项目(2021ZD0112302,2021ZD0112301),国家重点研发计划项目(2018YFC1900800–5),北京市自然科学基金项目(JQ19013),国家自然科学基金项目(62222301,61890930–5,62021003)资助.Supported by the National Key Research and Development Program of China(2021ZD0112302,2021ZD0112301,2018YFC1900800–5),the Beijing Natural Science Foundation(JQ19013)and the National Natural Science Foundation of China(62222301,61890930–5,62021003).第9期李梦花等:不对称约束多人非零和博弈的自适应评判控制1563性原理提供理论基础,神经网络作为函数近似结构提供实现手段,强化学习提供学习机制.值得注意的是, ADP方法具有强大的自学习能力,在处理非线性复杂系统的最优控制问题上具有很大的潜力[2–7].此外, ADP作为一种近似求解最优控制问题的新方法,已经成为智能控制与计算智能领域的研究热点.关于ADP的详细理论研究以及相关应用,读者可以参考文献[8–9].本文将基于ADP的动态系统优化控制统称为自适应评判控制.近年来,微分博弈问题在控制领域受到了越来越多的关注.微分博弈为研究多玩家系统的协作、竞争与控制提供了一个标准的数学框架,包括二人零和博弈、多人零和博弈以及多人非零和博弈等.在零和博弈问题中,控制输入试图最小化代价函数而干扰输入试图最大化代价函数.在非零和博弈问题中,每个玩家都独立地选择一个最优控制策略来最小化自己的代价函数.值得注意的是,零和博弈问题已经被广泛研究.在文献[10]中,作者提出了一种改进的ADP方法来求解多输入非线性连续系统的二人零和博弈问题.An等人[11]提出了两种基于积分强化学习的算法来求解连续时间系统的多人零和博弈问题.Ren等人[12]提出了一种新颖的同步脱策方法来处理多人零和博弈问题.然而,关于非零和博弈[13–14]的研究还很少.此外,控制约束在实际应用中也广泛存在.这些约束通常是由执行器的固有物理特性引起的,如气压、电压和温度.因此,为了确保被控系统的性能,受约束的系统需要被考虑.Zhang等人[15]发展了一种新颖的事件采样ADP方法来求解非线性连续约束系统的鲁棒最优控制问题.Huo等人[16]研究了一类非线性约束互联系统的分散事件触发控制问题.Yang和He[17]研究了一类具有不匹配扰动和输入约束的非线性系统事件触发鲁棒镇定问题.这些文献考虑的都是对称约束,而实际应用中,被控系统受到的约束也可能是不对称的[18–20],例如在污水处理过程中,需要通过氧传递系数和内回流量对溶解氧浓度和硝态氮浓度进行控制,而根据实际的运行条件,这两个控制变量就需要被限制在一个不对称约束范围内[20].因此,在控制器设计过程中,不对称约束问题将是笔者研究的一个方向.到目前为止,关于具有控制约束的微分博弈问题,有一些学者取得了相应的研究成果[12,21–23].但可以发现,具有不对称约束的多人非零和博弈问题还没有学者研究.同时,在多人非零和博弈问题中,相关的耦合Hamilton-Jacobi(HJ)方程是很难求解的.因此,本文针对一类连续时间非线性系统的不对称约束多人非零和博弈问题,提出了一种自适应评判控制方法来近似求解耦合HJ方程,从而获得被控系统的近似最优解.本文的主要贡献如下:1)首次将不对称约束应用到连续时间非线性系统的多人非零和博弈问题中;2)提出了一种新颖的非二次型函数来处理不对称约束问题,并且当系统状态为零时,最优控制策略是不为零的,这与以往不同;3)在学习期间,用单一评判网络结构代替了传统的执行–评判网络结构,并且提出了一种新的权值更新规则;4)利用Lyapunov方法证明了评判网络权值近似误差和系统状态的一致最终有界(uniformly ultimately bounded,UUB)稳定性.2问题描述考虑以下具有不对称约束的N–玩家连续时间非线性系统:˙x(t)=f(x(t))+N∑j=1g j(x(t))u j(t),(1)其中:x(t)∈Ω⊂R n是状态向量且x(0)=x0为初始状态,R n代表由所有n-维实向量组成的欧氏空间,Ω是R n的一个紧集;u j(t)∈T j⊂R m为玩家j在时刻t所选择的策略,且T j为T j={[u j1u j2···u jm]T∈R m:u j min u jl u j max, |u j min|=|u j max|,l=1,2,···,m},(2)其中:u jmin∈R和u j max∈R分别代表控制输入分量的最小界和最大界,R表示所有实数集.假设1非线性系统(1)是可控的,并且x=0是被控系统(1)的一个平衡点.此外,∀j∈N,f(x)和g j(x)是未知的Lipschitz函数且f(0)=0,其中集合N={1,2,···,N},N 2是一个正整数.假设2∀j∈N,g j(0)=0,且存在一个正常数b gj使∥g j(x)∥ b gj,其中∥·∥表示在R n上的向量范数或者在R n×m上的矩阵范数,R n×m代表由所有n×m维实矩阵组成的空间.注1假设1–3是自适应评判领域的常用假设,例如文献[6,13,19],是为了保证系统的稳定性以及方便后文中的稳定性证明,其中假设3出现在后文中的第3.2节.定义与每个玩家相关的效用函数为U i(x,U)=x T Q i x+N∑j=1S j(u j),i∈N,(3)其中U={u1,u2,···,u N}并且Q i是一个对称正定矩阵.此外,为了处理不对称约束问题,令S j(u j)为S j(u j)=2αj m∑l=1ujlβjtanh−1(z−βjαj)d z,(4)其中αj和βj分别为αj=u jmax−u j min2,βj=u jmax+u jmin2.(5)因此,与每个玩家相关的代价函数可以表示为J i(x0,U)=∞U i(x,U)dτ,i∈N,(6)1564控制理论与应用第40卷本文希望构建一个Nash均衡U∗={u∗1,u∗2,···,u∗N},来使以下不等式被满足:J i(u∗1,···,u∗i,···,u∗N)J i(u∗1,···,u i,···,u∗N),(7)其中i∈N.为了方便,将J i(x0,U)简写为J i(x0).于是,每个玩家的最优代价函数为J∗i (x0)=minu iJ i(x0,U),i∈N.(8)在本文中,如果一个控制策略集的所有元素都是可容许的,那么这个集合是可容许的.定义1(容许控制[24])如果控制策略u i(x)是连续的,u i(x)可以镇定系统(1),并且J i(x0)是有限的,那么它是集合Ω上关于代价函数(6)的可容许控制律,即u i(x)∈Ψ(Ω),i∈N,其中,Ψ(Ω)是Ω上所有容许控制律的集合.对于任意一个可容许控制律u i(x)∈Ψ(Ω),如果相关代价函数(6)是连续可微的,那么非线性Lyapu-nov方程为0=U i(x,U)+(∇J i(x))T(f(x)+N∑j=1g j(x)u j),(9)其中:i∈N,J i(0)=0,并且∇(·) ∂(·)∂x.根据最优控制理论,耦合HJ方程为0=minU H i(x,U,∇J∗i(x)),i∈N,(10)其中,Hamiltonian函数H i(x,U,∇J∗i(x))为H i(x,U,∇J∗i(x))=U i(x,U)+(∇J∗i (x))T(f(x)+N∑j=1g j(x)u j),(11)进而,由∂H i(x,U,∇J∗i(x))∂u i=0可得出最优控制律为u∗i (x)=−αi tanh(12αig Ti(x)∇J∗i(x))+¯βi,i∈N,(12)其中¯βi=[βiβi···βi]T∈R m.注2根据式(2)和式(5),能推导出βi=0,即¯βi=0,又根据式(12)可知u∗i(0)=0,i∈N.因此,为了保证x=0是系统(1)的平衡点,在假设2中提出了条件∀j∈N,g j(0)=0.将式(12)代入式(10),耦合HJ方程又能表示为(∇J∗i (x))T f(x)+N∑j=1((∇J∗i(x))T g j(x)¯βj)+x T Q i x−N∑j=1((∇J∗i(x))Tαj g j(x)tanh(A j(x)))+N∑j=1S j(−αj tanh(A j(x))+¯βj)=0,i∈N,(13)其中J∗i(0)=0并且A j(x)=12αjg Tj(x)∇J∗j(x).如果已知每个玩家的最优代价函数值,那么相关的最优状态反馈控制律就可以直接获得,也就是说式(13)是可解的.可是,式(13)这种非线性偏微分方程的求解是十分困难的.同时,随着系统维数的增加,存储量和计算量也随之以指数形式增加,也就是平常所说的“维数灾”问题.因此,为了克服这些弱点,在第3部分提出了一种基于神经网络的自适应评判机制,来近似每个玩家的最优代价函数,从而获得相关的近似最优状态反馈控制策略.3自适应评判控制设计3.1神经网络实现本节的核心是构建并训练评判神经网络,以得到训练后的权值,从而获得每个玩家的近似最优代价函数值.首先,根据神经网络的逼近性质[25],可将每个玩家的最优代价函数J∗i(x)在紧集Ω上表示为J∗i(x)=W Tiσi(x)+ξi(x),i∈N,(14)其中:W i∈Rδ是理想权值向量,σi(x)∈Rδ是激活函数,δ是隐含层神经元个数,ξi(x)∈R是重构误差.同时,可得出每个玩家的最优代价函数梯度为∇J∗i(x)=(∇σi(x))T W i+∇ξi(x),i∈N,(15)将式(15)代入式(12),有u∗i(x)=−αi tanh(B i(x)+C i(x))+¯βi,i∈N,(16)其中:B i(x)=12αig Ti(x)(∇σi(x))T W i∈R m,C i(x)=12αig Ti(x)∇ξi(x)∈R m.然后,将式(15)代入式(13),耦合HJ方程变为W Ti∇σi(x)f(x)+(∇ξi(x))T f(x)+x T Q i x+N∑j=1((W Ti∇σi(x)+(∇ξi(x))T)g j(x)¯βj)−N∑j=1(αj W Ti∇σi(x)g j(x)tanh(B j(x)+C j(x)))−N∑j=1(αj(∇ξi(x))T g j(x)tanh(B j(x)+C j(x)))+N∑j=1S j(−αj tanh(B j(x)+C j(x))+¯βj)=0,i∈N.(17)值得注意的是,式(14)中的理想权值向量W i是未知的,也就是说式(16)中的u∗i(x)是不可解的.因此,第9期李梦花等:不对称约束多人非零和博弈的自适应评判控制1565构建如下的评判神经网络:ˆJ∗i (x)=ˆW Tiσi(x),i∈N,(18)来近似每个玩家的最优代价函数,其中ˆW i∈Rδ是估计的权值向量.同时,其梯度为∇ˆJ∗i(x)=(∇σi(x))TˆW i,i∈N.(19)考虑式(19),近似的最优控制律为ˆu∗i(x)=−αi tanh(D i(x))+¯βi,i∈N,(20)其中D i(x)=12αig Ti(x)(∇σi(x))TˆW i.同理,近似的Hamiltonian可以写为ˆHi(x,ˆW i)=ˆW T i ϕi+x T Q i x+N∑j=1(ˆW Ti∇σi(x)g j(x)¯βj)−N ∑j=1(αjˆW Ti∇σi(x)g j(x)tanh(D j(x)))+N∑j=1S j(−αj tanh(D j(x))+¯βj),i∈N,(21)其中ϕi=∇σi(x)f(x).此外,定义误差量e i=ˆH i(x,ˆW i )−H i(x,U∗,∇J∗i(x))=ˆH i(x,ˆW i).为了使e i足够小,需要训练评判网络来使目标函数E i=12e Tie i最小化.在这里,本文采用的训练准则为˙ˆW i =−γi1(1+ϕTiϕi)2(∂E i∂ˆW i)=−γiϕi(1+ϕTiϕi)2e i,i∈N,(22)其中:γi>0是评判网络的学习率,(1+ϕT iϕi)2用于归一化操作.此外,定义评判网络的权值近似误差为˜Wi=W i−ˆW i.因此,有˙˜W i =γiφi1+ϕTiϕie Hi−γiφiφT i˜W i,i∈N,(23)其中:φi=ϕi(1+ϕTiϕi),e Hi=−(∇ξi(x))T f(x)是残差项.3.2稳定性分析本节的核心是通过利用Lyapunov方法讨论评判网络权值近似误差和闭环系统状态的UUB稳定性.这里,给出以下假设:假设3∥∇ξi(x)∥ b∇ξi ,∥∇σi(x)∥ b∇σi,∥e Hi∥ b e Hi,∥W i∥ b W i,其中:b∇ξi,b∇σi,b e Hi,b W i 都是正常数,i∈N.定理1考虑系统(1),如果假设1–3成立,状态反馈控制律由式(20)给出,且评判网络权值通过式(22)进行训练,则评判网络权值近似误差˜W i是UUB 稳定的.证选取如下的Lyapunov函数:L1(t)=N∑i=1(12˜W Ti˜Wi)=N∑i=1L1i(t),(24)计算L1i(t)沿着式(23)的时间导数,即˙L1i(t)=γi˜W Tiφi1+ϕTiϕie Hi−γi˜W TiφiφTi˜Wi,i∈N,(25)利用不等式¯X T¯Y12∥¯X∥2+12∥¯Y∥2(注:¯X和¯Y都是具有合适维数的向量),并且考虑1+ϕTiϕi 1,能得到˙L1i(t)γi2(∥φTi˜Wi∥2+∥e Hi∥2)−γi˜W TiφiφTi˜Wi=−γi2˜W TiφiφTi˜Wi+γi2∥e Hi∥2,i∈N.(26)根据假设3,有˙L1i(t) −γi2λmin(φiφTi)∥˜W i∥2+γi2b2e Hi,i∈N,(27)其中λmin(·)表示矩阵的最小特征值.因此,当不等式∥˜W i∥>√b2e Hiλmin(φiφTi),i∈N(28)成立时,有˙L1i(t)<0.根据标准的Lyapunov定理[26],可知评判网络权值近似误差˜W i是UUB稳定的.证毕.定理2考虑系统(1),如果假设1–3成立,状态反馈控制律由式(20)给出,且评判网络权值通过式(22)进行训练,则系统状态x(t)是UUB稳定的.证选取如下的Lyapunov函数:L2i(t)=J∗i(x),i∈N.(29)计算L2i(t)沿着系统˙x=f(x)+N∑j=1g j(x)ˆu∗j的时间导数,即˙L2i(t)=(∇J∗i(x))T(f(x)+N∑j=1g j(x)ˆu∗j)=(∇J∗i(x))T(f(x)+N∑j=1g j(x)u∗j)+N∑j=1((∇J∗i(x))T g j(x)(ˆu∗j−u∗j)),i∈N.(30)考虑式(13),有˙L2i(t)=−x T Q i x−N∑j=1S j(u∗j)+N∑j=1((∇J∗i(x))T g j(x)(ˆu∗j−u∗j))Σi,i∈N,(31)1566控制理论与应用第40卷利用不等式¯XT ¯Y 12∥¯X ∥2+12∥¯Y ∥2,并且考虑式(15)–(16)(20),可得Σi 12N ∑j =1∥−αj tanh (D j (x ))+αj tanh (F j (x ))∥2+12N ∑j =1∥g Tj (x )((∇σi (x ))T W i +∇ξi (x ))∥2,i ∈N ,(32)其中F j (x )=B j (x )+C j (x ).然后,利用不等式∥¯X+¯Y∥2 2∥¯X ∥2+2∥¯Y ∥2,有Σi N ∑j =1(∥αj tanh (D j (x ))∥2+∥αj tanh (F j (x ))∥2)+N ∑j =1∥g Tj (x )(∇σi (x ))T W i ∥2+N ∑j =1∥g T j (x )∇ξi (x )∥2,i ∈N ,(33)其中D j (x )∈R m ,F j (x )∈R m 分别被表示为[D j 1(x )D j 2(x )···D jm (x )]T 和[F j 1(x )F j 2(x )···F jm (x )]T .易知,∀θ∈R ,tanh 2θ 1.因此,有∥tanh (D j (x ))∥2=m ∑l =1tanh 2(D jl (x )) m,(34)∥tanh (F j (x ))∥2=m ∑l =1tanh 2(F jl (x )) m.(35)同时,根据假设2–3,有Σi N ∑j =1(2α2j m +b 2g j b 2∇σi b 2W i +b 2g j b 2∇ξi ),i ∈N ,(36)根据式(2)(4)–(5),可知S j (u ∗j ) 0.于是,有˙L2i (t ) −λmin (Q i )∥x ∥2+ϖi ,i ∈N ,(37)其中ϖi =N ∑j =1(2α2j m +b 2g j b 2∇σi b 2W i +b 2g j b 2∇ξi ).因此,根据式(37)可知,当不等式∥x ∥>√ϖiλmin (Q i )成立时,有˙L2i (t )<0.即,如果x (t )满足下列不等式:∥x ∥>max {√ϖ1λmin (Q 1),···,√ϖNλmin (Q N )},(38)则,∀i ∈N ,都有˙L 2i (t )<0.同理,可得闭环系统状态x (t )也是UUB 稳定的.证毕.4仿真结果考虑如下的3–玩家连续时间非线性系统:˙x =[−1.2x 1+1.5x 2sin x 20.5x 1−x 2]+[01.5sin x 1cos x 1]u 1(x )+[1.2sin x 1cos x 2]u 2(x )+[01.1sin x 2]u 3(x ),(39)其中:x (t )=[x 1x 2]T ∈R 2是状态向量,u 1(x )∈T 1={u 1∈R :−1 u 1 2},u 2(x )∈T 2={u 2∈R :−0.2 u 2 1}和u 3(x )∈T 3={u 3∈R :−0.4 u 3 0.8}是控制输入.令Q 1=2I 2,Q 2=1.8I 2,Q 3=0.3I 2,其中I 2代表2×2维单位矩阵.同时,根据式(5)可知,α1=1.5,β1=0.5,α2=0.6,β2=0.4,α3=0.6,β3=0.2.因此,与每个玩家相关的代价函数可以表示为J i (x 0)= ∞0(x TQ i x +3∑j =1S j (u j ))d τ,i =1,2,3,(40)其中S j (u j )=2αju jβj tanh −1(z −βjαj)d z =2αj (u j −βj )tanh −1(u j −βjαj)+α2j ln (1−(u j −βj )2α2j).(41)然后,本文针对系统(39)构建3个评判神经网络,每个玩家的评判神经网络权值分别为ˆW1=[ˆW 11ˆW 12ˆW13]T ,ˆW 2=[ˆW 21ˆW 22ˆW 23]T ,ˆW 3=[ˆW 31ˆW 32ˆW33]T ,激活函数被定义为σ1(x )=σ2(x )=σ3(x )=[x 21x 1x 2x 22]T,且隐含层神经元个数为δ=3.此外,系统初始状态取x 0=[0.5−0.5]T ,每个评判神经网络的学习率分别为γ1=1.5,γ2=0.8,γ3=0.2,且每个评判神经网络的初始权值都在0和2之间选取.最后,引入探测噪声η(t )=sin 2(−1.2t )cos(0.5t )+cos(2.4t )sin 3(2.4t )+sin 5t +sin 2(1.12t )+sin 2t ×cos t +sin 2(2t )cos(0.1t ),使得系统满足持续激励条件.执行学习过程,本文发现每个玩家的评判神经网络权值分别收敛于[6.90912.99046.6961]T ,[4.89012.23475.2062]T ,[1.79450.33212.4583]T .在60个时间步之后去掉探测噪声,每个玩家的评判网络权值收敛过程如图1–3所示.然后,将训练好的权值代入式(20),能得到每个玩家的近似最优控制律,将其应用到系统(39),经过10个时间步之后,得到的状态轨迹和控制轨迹分别如图4–5所示.由图4可知,系统状态最终收敛到了平衡点.由图5可知,每个玩家的控制轨迹都没有超出预定的边界,并且可以观察到u 1,u 2和u 3分别收敛于0.5,0.4和0.2.综上所述,仿真结果验证了所提方法的有效性.第9期李梦花等:不对称约束多人非零和博弈的自适应评判控制1567䇴 㖁㔌U / s图1玩家1的评判网络权值收敛过程Fig.1Convergence process of the critic network weights forplayer1䇴 㖁㔌U / s图2玩家2的评判网络权值收敛过程Fig.2Convergence process of the critic network weights forplayer2﹣䇴 㖁㔌U / s图3玩家3的评判网络权值收敛过程Fig.3Convergence process of the critic network weights forplayer 35结论本文首次将不对称约束应用到连续时间非线性系统的多人非零和博弈问题中.首先,获得了最优状态反馈控制律和耦合HJ 方程,并且为了解决不对称约束问题,建立了一种新的非二次型函数.值得注意的是,当系统状态为零时,最优控制策略是不为零的.其次,由于耦合HJ 方程不易求解,提出了一种基于神经网络的自适应评判算法来近似每个玩家的最优代价函数,从而获得相关的近似最优控制律.在实现过程中,用单一评判网络结构代替了经典的执行–评判结构,并且建立了一种新的权值更新规则.然后,利用Lyap-unov 理论讨论了评判网络权值近似误差和系统状态的UUB 稳定性.最后,仿真结果验证了所提算法的可行性.在未来的工作中,会考虑将事件驱动机制引入到连续时间非线性系统的不对称约束多人非零和博弈问题中,并且将该研究内容应用到污水处理系统中也是笔者的一个重点研究方向.﹣0.5﹣0.4﹣0.3﹣0.2﹣0.10.00.10.20.00.10.20.30.40.5(U )Y 1(U )Y 2图4系统(39)的状态轨迹Fig.4State trajectory of the system (39)0.00.51.01.52.00.00.20.40.60.81.01.200.012345678910﹣0.40.4﹣0.20.2(U )V 3(U )V 2(U )V 1U / s 012345678910U / s 012345678910U / s (c)(b)(a)(U )V 1(U )V 2(U )V 3图5系统(39)的控制轨迹Fig.5Control trajectories of the system (39)1568控制理论与应用第40卷参考文献:[1]WERBOS P J.Beyond regression:New tools for prediction andanalysis in the behavioral sciences.Cambridge:Harvard Universi-ty,1974.[2]HONG Chengwen,FU Yue.Nonlinear robust approximate optimaltracking control based on adaptive dynamic programming.Control Theory&Applications,2018,35(9):1285–1292.(洪成文,富月.基于自适应动态规划的非线性鲁棒近似最优跟踪控制.控制理论与应用,2018,35(9):1285–1292.)[3]CUI Lili,ZHANG Yong,ZHANG Xin.Event-triggered adaptive dy-namic programming algorithm for the nonlinear zero-sum differential games.Control Theory&Applications,2018,35(5):610–618.(崔黎黎,张勇,张欣.非线性零和微分对策的事件触发自适应动态规划算法.控制理论与应用,2018,35(5):610–618.)[4]WANG D,HA M,ZHAO M.The intelligent critic framework foradvanced optimal control.Artificial Intelligence Review,2022,55(1): 1–22.[5]WANG D,QIAO J,CHENG L.An approximate neuro-optimal solu-tion of discounted guaranteed cost control design.IEEE Transactions on Cybernetics,2022,52(1):77–86.[6]YANG X,HE H.Adaptive dynamic programming for decentralizedstabilization of uncertain nonlinear large-scale systems with mis-matched interconnections.IEEE Transactions on Systems,Man,and Cybernetics:Systems,2020,50(8):2870–2882.[7]ZHAO B,LIU D.Event-triggered decentralized tracking control ofmodular reconfigurable robots through adaptive dynamic program-ming.IEEE Transactions on Industrial Electronics,2020,67(4): 3054–3064.[8]WANG Ding.Research progress on learning-based robust adaptivecritic control.Acta Automatica Sinica,2019,45(6):1037–1049.(王鼎.基于学习的鲁棒自适应评判控制研究进展.自动化学报, 2019,45(6):1037–1049.)[9]ZHANG Huaguang,ZHANG Xin,LUO Yanhong,et al.An overviewof research on adaptive dynamic programming.Acta Automatica Sini-ca,2013,39(4):303–311.(张化光,张欣,罗艳红,等.自适应动态规划综述.自动化学报, 2013,39(4):303–311.)[10]L¨U Yongfeng,TIAN Jianyan,JIAN Long,et al.Approximate-dynamic-programming H∞controls for multi-input nonlinear sys-tem.Control Theory&Applications,2021,38(10):1662–1670.(吕永峰,田建艳,菅垄,等.非线性多输入系统的近似动态规划H∞控制.控制理论与应用,2021,38(10):1662–1670.)[11]AN P,LIU M,WAN Y,et al.Multi-player H∞differential gameusing on-policy and off-policy reinforcement learning.The16th In-ternational Conference on Control and Automation.Electr Network: IEEE,2020,10:1137–1142.[12]REN H,ZHANG H,MU Y,et al.Off-policy synchronous iterationIRL method for multi-player zero-sum games with input constraints.Neurocomputing,2020,378:413–421.[13]LIU D,LI H,WANG D.Online synchronous approximate optimallearning algorithm for multiplayer nonzero-sum games with unknown dynamics.IEEE Transactions on Systems,Man,and Cybernetics: Systems,2014,44(8):1015–1027.[14]V AMVOUDAKIS K G,LEWIS F L.Non-zero sum games:Onlinelearning solution of coupled Hamilton-Jacobi and coupled Riccati equations.IEEE International Symposium on Intelligent Control.Denver,CO,USA:IEEE,2011,9:171–178.[15]ZHANG H,ZHANG K,XIAO G,et al.Robust optimal controlscheme for unknown constrained-input nonlinear systems via a plug-n-play event-sampled critic-only algorithm.IEEE Transactions on Systems,Man,and Cybernetics:Systems,2020,50(9):3169–3180.[16]HUO X,KARIMI H R,ZHAO X,et al.Adaptive-critic design fordecentralized event-triggered control of constrained nonlinear inter-connected systems within an identifier-critic framework.IEEE Trans-actions on Cybernetics,2022,52(8):7478–7491.[17]YANG X,HE H.Event-triggered robust stabilization of nonlin-ear input-constrained systems using single network adaptive critic designs.IEEE Transactions on Systems,Man,and Cybernetics:Sys-tems,2020,50(9):3145–3157.[18]WANG L,CHEN C L P.Reduced-order observer-based dynamicevent-triggered adaptive NN control for stochastic nonlinear systems subject to unknown input saturation.IEEE Transactions on Neural Networks and Learning Systems,2021,32(4):1678–1690.[19]YANG X,ZHU Y,DONG N,et al.Decentralized event-driven con-strained control using adaptive critic designs.IEEE Transactions on Neural Networks and Learning Systems,2022,33(10):5830–5844.[20]WANG D,ZHAO M,QIAO J.Intelligent optimal tracking withasymmetric constraints of a nonlinear wastewater treatment system.International Journal of Robust and Nonlinear Control,2021,31(14): 6773–6787.[21]LI M,WANG D,QIAO J,et al.Neural-network-based self-learningdisturbance rejection design for continuous-time nonlinear con-strained systems.Proceedings of the40th Chinese Control Confer-ence.Shanghai,China:IEEE,2021,7:2179–2184.[22]SU H,ZHANG H,JIANG H,et al.Decentralized event-triggeredadaptive control of discrete-time nonzero-sum games over wireless sensor-actuator networks with input constraints.IEEE Transactions on Neural Networks and Learning Systems,2020,31(10):4254–4266.[23]YANG X,HE H.Event-driven H∞-constrained control using adap-tive critic learning.IEEE Transactions on Cybernetics,2021,51(10): 4860–4872.[24]ABU-KHALAF M,LEWIS F L.Nearly optimal control laws for non-linear systems with saturating actuators using a neural network HJB approach.Automatica,2005,41(5):779–791.[25]HORNIK K,STINCHCOMBE M,WHITE H.Universal approxima-tion of an unknown mapping and its derivatives using multilayer feed-forward networks.Neural Networks,1990,3(5):551–560.[26]LEWIS F L,JAGANNATHAN S,YESILDIREK A.Neural NetworkControl of Robot Manipulators and Nonlinear Systems.London:Tay-lor&Francis,1999.作者简介:李梦花博士研究生,目前研究方向为自适应动态规划、智能控制,E-mail:*********************;王鼎教授,博士生导师,目前研究方向为智能控制、强化学习,E-mail:*****************.cn;乔俊飞教授,博士生导师,目前研究方向为智能计算、智能优化控制,E-mail:***************.cn.。

Bethe Ansatz Solutions and Excitation Gap of the Attractive Bose-Hubbard Model

a r X i v :c o n d -m a t /0108314v 1 [c o n d -m a t .s t a t -m e c h ] 20 A u g 2001Bethe Ansatz Solutions and Excitation Gap of the Attractive Bose-Hubbard ModelDeok-Sun Lee and Doochul KimSchool of Physics,Seoul National University,Seoul 151-747,KoreaThe energy gap between the ground state and the first excited state of the one-dimensional attractive Bose-Hubbard Hamiltonian is investigated in connection with directed polymers in random media.The excitation gap ∆is obtained by exact diagonalization of the Hamiltonian in the two-and three-particle sectors and also by an exact Bethe Ansatz solution in the two-particle sector.The dynamic exponent z is found to be 2.However,in the intermediate range of the size L where UL ∼O (1),U being the attractive interaction,the effective dynamic exponent shows an anomalous peak reaching high values of 2.4and 2.7for the two-and the three-particle sectors,respectively.The anomalous behavior is related to a change in the sign of the first excited-state energy.In the two-particle sector,we use the Bethe Ansatz solution to obtain the effective dynamic exponent as a function of the scaling variable UL/π.The continuum version,the attractive delta-function Bose-gas Hamiltonian,is integrable by the Bethe Ansatz with suitable quantum numbers,the distributions of which are not known in general.Quantum numbers are proposed for the first excited state and are confirmed numerically for an arbitrary number of particles.I.INTRODUCTIONThe dynamics of many simple non-equilibrium sys-tems are often studied through corresponding quantum Hamiltonians.Examples are the asymmetric XXZ chain Hamiltonian and the attractive Bose-Hubbard Hamilto-nian for the single-step growth model [1]and the directed polymers in random media (DPRM)[2],respectively.The single-step growth model is a Kardar-Parisi-Zhang (KPZ)universality class growth model where the inter-face height h (x,t )grows in a stochastic manner under the condition that h (x ±1,t )−h (x,t )=±1.The process is also called the asymmetric exclusion process (ASEP)in a different context.The evolution of the probability distri-bution for h (x,t )is generated by the asymmetric XXZ chain Hamiltonian [3].The entire information about the dynamics is coded in the generating function e αh (x,t ) .Its time evolution,in turn,is given by the modified asym-metric XXZ chain Hamiltonian [4–6],H XXZ (α)=−L i =1e 2α/L σ−i σ+i +1+12L i =1(b i b †i +1+b †i b i +1−2)−UL i =1b †ib i (b †ib i −1)4Lρ(1−ρ)and −n√4Lρ(1−ρ)≫1and the density of particles is fi-nite in the limit L →∞,∆(α)behaves as ∆(α)∼L −1.However,when α∆(α)∼L−3/2[3,11].The dynamic exponent z=3/2is a characteristic of the dynamic universality class of the KPZ-type surface growth.When the number of par-ticles isfinite and the density of particles is very low, it is known that∆(α)∼L−2[12].However,whenα<0,which corresponds to the ferromagnetic phase, most Bethe Ansatz solutions are not available althoughthe Bethe Ansatz equations continue to hold.Asαbe-comes negative,the quasi-particle momenta appearing inthe Bethe Ansatz equations become complex,so solutions are difficult to obtain analytically.The attractive Bose-Hubbard Hamiltonian is expected to have some resemblance to the ferromagnetic phaseof the asymmetric XXZ chain Hamiltonian consider-ing the equivalence ofαand−n.The equivalence isidentified indirectly by comparing the two scaling vari-ablesα LU under the relation U= 4ρ(1−ρ)or the two generating functions exp(αh(x,t) and Z(x,t)n under the relation Z(x,t)=e−h(x,t).In contrast to the asymmetric XXZ chain Hamiltonian,theBose-Hubbard Hamiltonian does not satisfy the Bethe Ansatz except in the two-particle sector[13].Instead, the attractive delta-function Bose-gas Hamiltonian,H D(n)=−1∂x2i−Ui<jδ(x i−x j),(4)which is the continuum version of the attractive Bose-Hubbard Hamiltonian,is known to be integrable by the Bethe Ansatz.The attractive delta-function Bose gas has been studied in Refs.[14]and[15].The ground-state energy is obtained from the Bethe Ansatz solution by us-ing the symmetric distribution of the purely imaginary quasi-particle momenta.However,the structure of the energy spectra is not well known for the same reason as in the asymmetric XXZ chain Hamiltonian withα<0. The unknown energy spectra itself prevents one from un-derstanding the dynamics of DPRM near the stationary state.In this paper,we discuss in Section II the distribu-tion of the quantum numbers appearing in the Bethe Ansatz equation for thefirst excited state of the attrac-tive delta-function Bose-gas Hamiltonian,the knowledge of which is essential for solving the Bethe Ansatz equa-tion.In Section III,the excitation gap of the attractive Bose-Hubbard Hamiltonian with a small number of par-ticles is investigated through the exact diagonalization method.We show that the gap decays as∆∼L−2,i.e., z=2,but that the exponent becomes anomalous when U∼L−1.The emergence of the anomalous exponent is explained in connection with the transition of thefirst excited state from a positive energy state to a negative energy state.The Bethe Ansatz solutions in the two-particle sector show how the behavior of the gap varies with the interaction.We give a summary and discussion in Section IV.II.QUANTUM NUMBER DISTRIBUTION FOR THE FIRST EXCITED STATEIn this section,we study the Bethe Ansatz solutions for the ground state and thefirst excited state of the attrac-tive delta-function Bose-gas Hamiltonian.The eigenstate of H D(n),Eq.(4),is of the formφ(x1,x2,...,x n)= P A(P)exp(ik P1x1+ik P2x2+···+ik P n x n),(5)where P is a permutation of1,2,...,n and x1≤x2≤...≤x n with no three x’s being equal.The quasi-particle momenta k j’s are determined by solving the Bethe Ansatz equations,k j L=2πI j+ l=jθ(k j−k l2+j,(j=1,2,...,n),(7)and the quasi-particle momenta are distributed symmet-rically on the imaginary axis in the complex-k plane. Care should be taken when dealing with thefirst excited state.For the repulsive delta-function Bose-gas Hamilto-nian,where U is replaced by−U in Eq.(4),the quantum numbers for one of thefirst excited states areI j=−n+12.(8)However,for the attractive case,by following the move-ment of the momenta as U changes sign,wefind that the quantum numbers for thefirst excited state should be given byI j=−n−12(=I1).(9)That is,the two quantum numbers I1and I n become the same.Such a peculiar distribution of I j’s does not ap-pear in other Bethe Ansatz solutions such as those for the XXZ chain Hamiltonian or the repulsive delta-function Bose-gas Hamiltonian.We remark that even though the two I j’s are the same,all k j’s are distinct;otherwise,the wavefunction vanishes.Such a distribution of quan-tum numbers is confirmed by the consistency between the energies obtained by diagonalizing the Bose-HubbardHamiltonian exactly and those obtained by solving the Bethe Ansatz equations with the above quantum num-bers for very weak interactions,for which the two Hamil-tonians possess almost the same energy spectra.When there is no interaction(U=0),all quasi-particlemomenta,k j’s,are zero for the ground state while for thefirst excited state,all the k j’s are zero except thelast one,k n=2π/L.In the complex-k plane,as the very weak repulsive interaction is turned on,the n−1momenta are shifted infinitesimally from k=0withk1<k2<···<k n−1,and the n th momentum is shifted infinitesimally to the left from k=2π/L.All the mo-menta remain on the real axis.When the interaction is weakly attractive,the n−1momenta become complexwith Im k1<Im k2<···<Im k n−1and Re k j≃0for j=1,2,...,n−1,and the n th momentum remains on thereal axis,but is shifted to the left.Figure1shows the dis-tribution of the quantum numbers and the quasi-particlemomenta in the presence of a very weak attractive in-teraction.The quasi-particle momenta are obtained by solving Eq.(6).Knowledge of the distribution of the quantum num-bers is essential for solving the Bethe Ansatz equations of the attractive delta-function Bose-gas Hamiltonian.For the original attractive Bose-Hubbard Hamiltonian,the Bethe Ansatz solutions are the exact solutions for the two-particle sector only,but are good approximate so-lutions in other sectors provided the density is very low and the interaction is very weak.This is because the Bethe Ansatz for the Bose-Hubbard Hamiltonian fails once states with sites occupied by more than three parti-cles are included.Thus,for the sectors with three or more particles,the Bethe Ansatz solutions may be regarded as approximate eigenstates provided states with more than three particles at a site do not play an important role in the eigenfunctions.In Ref.[13],it is shown that the error in the Bethe Ansatz due to multiply-occupied sites (occupied by more than three particles)is proportional to U2,where U(>0)in Ref.[13]corresponds to−U in Eq.(2).This applies to the attractive interaction case also.For the repulsive Bose-Hubbard Hamiltonian,the Bethe Ansatz is a good approximation when the density is low and the interaction is strong because the strong re-pulsion prevents many particles from occupying the same site[16].For the attractive Bose-Hubbard Hamiltonian, the Bethe Ansatz is good when the density is low and the interaction is weak because a weak attraction is better for preventing many particles from occupying the same site and because the error is proportional to U2.III.POWER-LA W DEPENDENCE ANDANOMALOUS EXPONENTWe are interested in the scaling limit L→∞with the scaling variable n√byE 0=−4sinh 2 κ2Lcosh2q 2L sinh2q2sinh κ−U,(12)andqL =logU +2cos(πU −2cos(π2s κ−s U,(14)which gives s κ≃1.151.When the size of the system L is increased by δL with U =U∗,the changes of κand q ,δκand δq ,are,from Eqs.(12)and (13),δκ=−πs κ(4s κ2−s U 2)L 2≡−πΓδL(4/π)s U −s U 2+4δLL 2.(15)The perturbative expansion ∆(L +δL )≃∆(L )(1−z (δL/L )),under the assumption that ∆(L )∼L −z ,gives the value of z effat U ∗:z eff=21+s κΓ+Σlog((L −1)/(L +1))(17)by using the solutions of Eqs.(12)and (13)for sufficiently large L .As discussed above,the exponent z effshows an anomalous peak near U =U ∗or UL/π=s U and ap-proaches 2.0as UL/π→0or ∞.Figure 6shows a plot of z effversus the scaling variable UL/πat L =10000.IV.SUMMARY AND DISCUSSIONAs the asymmetric XXZ chain generates the dy-namics of the single-step growth model,the attractive Bose-Hubbard Hamiltonian governs the dynamics of the DPRM.We studied the attractive Bose-Hubbard Hamil-tonian and its continuum version,the attractive delta-function Bose-gas Hamiltonian concentrating on the be-havior of the excitation gap,which is related to the char-acteristics of DPRM relaxing into the stationary state.For the attractive delta-function Bose gas Hamiltonian,The quantum numbers for the first excited state in the Bethe Ansatz equation are found for the attractive delta-function Bose gas Hamiltonian,and the distribution of the quasi-particle momenta is discussed in the presence of a very weak attractive interaction.Our result is the start-ing point for a further elucidation of the Bethe Ansatz solutions.We show that the excitation gap depends on the size of the system as a power law,∆∼L −z ,and that the exponent z can be calculated by using an exact diag-onalization of the attractive Bose-Hubbard Hamiltonian in the two-and the three-particle sectors and by using the Bethe Ansatz solution in the two-particle sector.The exponent z is 2.0.However,for the intermediate region where UL ∼O (1),the effective exponent z effshows a peak.The equivalence of the differential equations govern-ing the single-step growth model and DPRM implies some inherent equivalence in the corresponding Hamil-tonians.The power-law behavior of the excitation gap,∆∼L −2,for the attractive Bose-Hubbard Hamiltonian with a very weak interaction is the same as that for the asymmetric XXZ chain Hamiltonian with a small num-ber of particles,which is expected considering the rela-tion U =4ρ(1−ρ).The fact that the excitation gap behaves anomalously for U ∼L −1implies the possibility of an anomalous dynamic exponent z for a finite scaling variable n√[1]M.Plischke,Z.Racz,and D.Liu,Phys.Rev.B 35,3485(1987).[2]M.Kardar,Nucl.Phys.B 290[FS20],582(1987).[3]L.H.Gwa and H.Spohn,Phys.Rev.A 46,844(1992).[4]B.Derrida and J.L.Lebowitz,Phys.Rev.Lett.80,209(1998).[5]D.-S.Lee and D.Kim,Phys.Rev.E 59,6476(1999).[6]B.Derrida and C.Appert,J.Stat.Phys.94,1(1999).[7]J.Krug and H.Spohn,in Solids Far from Equilibrium ,edited by C.Godr´e che (Cambridge University Press,Cambridge,1991),p.412.[8]B.Derrida and K.Mallick,J.Phys.A 30,1031(1997).[9]S.-C.Park,J.-M.Park,and D.Kim,unpublished.[10]E.Brunet and B.Derrida,Phys.Rev.E 61,6789(2000).[11]D.Kim,Phys.Rev.E 52,3512(1995).[12]M.Henkel and G.Sch¨u tz,Physica A 206,187(1994).[13]T.C.Choy and F.D.M.Haldane,Phys.Lett.90A ,83(1982).[14]E.H.Lieb and W.Liniger,Phys.Rev.130,1605(1963).[15]J.G.Muga and R.F.Snider,Phys.Rev.A 57,3317(1998).[16]W.Krauth,Phys.Rev.B 44,9772(1991).(a)ω-0.10.1-0.50.5(b)Re k Im k 0FIG.1.For the first excited state,(a)the quantum num-bers I j ’s are depicted in the complex-ωplane with ω=e 2πiI/L and (b)the quasi-particle momenta k j ’s are shown in the complex-k plane.Here,the size of the system L is 20,the number of particles n is 10,and the attractive interaction U is 0.0025.The filled circle in (a)is where the two quantum numbers overlap.0.5 1102030EL n =2 U =0.05ground state first excited state0.5 1102030EL n =2 U =0.5ground state first excited state-3.4-3.3-3.2 102030EL n =2 U =5ground state first excited state0.5 11020 30EL n =3 U =0.05ground state first excited state-0.5 0 0.5 1020 30ELn =3 U =0.5ground state first excited state-12.17-12.16-12.15 1020 30ELn =3 U =5ground state first excited stateFIG.2.Ground-state energies and first excited-state ener-gies are plotted versus the size of the system L (4≤L ≤30)for U =0.05,0.5,and 5in the two-and the three-particle sectors.The dotted line represents E =0.For all values of U and L ,the ground-state energy is negative.On the other hand,when U =0.5,the excited-state energy becomes nega-tive near L ≃14in the two-particle sector and L ≃6in the three-particle sector.The signs of the excited-state energies for U =0.05and 5do not change in the range of L shown here.0.0010.010.1110102030∆LU=0.05U=0.5U=5FIG.3.Log-log plot of the excitation gaps (∆)versus the size of the system (L )in the two-particle sector.Data for U =0.05and 5approach straight lines with slope z =2.0,but those for U =0.5show a strong crossover before approach-ing the asymptotic behavior.The solid line for U =0.5is that fitted in the range 14≤L ≤18,and shows an effective z ≃2.4.0.00010.001 0.010.1110102030∆LU=0.05U=0.5U=5FIG.4.Same as in Fig.3,but for the three-particle sec-tor.The fitted solid line used the data for 8≤L ≤12,and has a slope of approximately 2.7.(a)k (b)k FIG.5.Distributions of the quasi-particle momenta,k j ’s,for the ground state (filled circles)and the first excited state (open circles)are shown in the complex-k plane for n =2.The size of the system L is 100and the interaction U is (a)0.001and (b)0.1.22.22.4s U510z e f fU L/πFIG.6.Effective exponent z effin the two-particle sector versus the scaling variable UL/πat L =10000.The interac-tion U varies from 0.0001to 0.001.At UL/π=s U ≃2.181,z eff≃2.401.。

SPH真实感流体交互模拟的改进算法

第41卷第3期 2019年6月武汉工程大学学报Journal of Wuhan Institute of TechnologyVol.41 No.3Jun.2019文章编号:1674 - 2869(2019)03 - 0303 - 04SPH真实感流体交互模拟的改进算法程志宇h2,徐国庆”’2,张岚斌K2,许犇1'21.武汉工程大学计算机科学与工程学院,湖北武汉430205;2.智能机器人湖北省重点实验室(武汉工程大学),湖北武汉430205摘要:针对目前流体仿真中存在的模拟效率低及模拟交互的真实感不足等问题,提出一种基于光滑粒子流体动力学的流体模拟改进算法。

首先,采用光滑粒子流体动力学方法进行粒子系统建模,通过矫正压力及速度场保证流体求解方程的精确性和稳定性;然后通过简化流体计算模型,完成流体表面建模,提高流体表面渲染速度;最后使用硬件加速算法实现流体模拟的快速渲染,提高流体的真实感和交互的实时性。

实验结果表明,该算法能够明显提升流体渲染的真实感,减小计算复杂性。

大规模粒子实时模拟帧率达到20帧/s,实现了较为真实的交互应用。

关键词:流体模拟;光滑粒子流体动力学方法;硬件加速中图分类号:T P391 文献标识码:A d o i:10. 3969/j. issn. 1674-2869. 2019. 03. 018Improved Algorithm for Realistic Fluid Interactive Simulation Based onSmoothed Particle HydrodynamicsC H E N G Zhiyu u\X U Guoqing m'\Z H A N G Lanbinx\X U Ben121.School of Computer Science and Engineering, Wuhan Institute of Technology, Wuhan 430205, China;2. Hubei Key Laboratory of Intelligent Robot(Wuhan Institute of Technology),W u h a n430205, ChinaAbstract:T o solve the low efficiency and reality in the real fluid simulation,this paper presents an improved smoothed particle hydrodynamics m o v e m e n t simulation algorithm.Firstly,the particle system was modeled by smoothed particle hydrodynamics m e t h o d.T h e accuracy and stability of the fluid solution equation was improved by correcting the pressure and velocity fields.Secondly,the water surface w as modeled and the rendering speedof the fluid surface was optimized by simplifying the fluid particles calculation.Finally, acceleration algorithm was used to achieve faster fluid rendering.T h e experimental results algorithm can significantly enhance the reality of fluid rendering and reduce the computational large-scale particle real-time simulation,the frame rate reaches 20 frames per s e c o n d,which interactive application.the hardware show that the complexity.In realizes a realKeywords:fluid simulation;smoothed particle hydrodynamics;hardware acceleration真实感流体模拟是计算机图像学领域中的研 究热点,不管是在电视特效和广告、电子游戏亦或 是军用作战平台仿真、虚拟医学等领域中都有着 广泛的应用。

Abstract Particle Dynamics in LEP at Very High Energy

Now
1z
t
Abstract
Beam energy Radiation loss Damping time Energy spread Quantum excitation Emittance
E=GeV U0 =GeV x =T0 103 " 2 109 4 " T0 = x =nm
LEP1 LEP2
Particle Dynamics in LEP at Very High Energy
F. Barbarin,

F.C. Iselin, CERN
J.M. Jowett
CH-1211 Geneva 23
As the beam energy of LEP is increased up to 90 GeV LEP2 and beyond, the single-particle dynamics is ever more strongly in uenced by the emission of synchrotron radiation. The program MAD has recently been modi ed to simulate individual photon emissions in magnetic elements or the classical component. E ects of radiation damping and quantum uctuations the 6-dimensional sawtooth" closed orbit, normal modes, emittances, etc. emerge in a completely natural way. Analysis of tracked orbits has changed the understanding of the physical e ects determining the dynamic aperture of LEP2. Non-resonant radiative beta-synchrotron coupling and tune-dependences on betatron amplitudes play roles commensurate with those of the chromatic e ects. Resonances and coherent excitations generate new attractors of the underlying deterministic dissipative system. Phase space distribution functions on these can be computed by including the quantum uctuations. The energy of LEP will shortly be doubled with the addition of a large super-conducting RF system to compensate a synchrotron radiation energy loss per turn of the order of 2 of the beam energy. This will give rise to signi cant energy sawtoothing" e ects which are important even at the level of closed-orbit and linear optics 1, 2 . From the values of the dimensionless parameters characterising damping and quantum excitation see Table 1, we can say that LEP2 like TRISTAN will be a very high" energy ring. In the formulation of 3 , to which we refer for details, the equations of motion of an electron or positron are @H @H x0 = @p ; p0x = , @H , PpX cs @p ; @x x 02 x @H @H y0 = @p ; p0y = , @H , PpX cs @p ; 1 2 @y zt0 = @H ; p0t = , @H + PpX cs @H ; @pt @zt 0 2 @pt where primes denote derivatives with respect to azimuth s and X = x; y; zt; px; py ; = p , p0 =p0 are the particle's canonical coordinates relative to a closed reference curve1 all momenta are de ned in units of p0 . External electromagnetic elds are described in the Hamiltonian H . The
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bInstitute for Theoretical Physics, University of Amsterdam Valckenierstraat 65, 1018 XE Amsterdam, the Netherlands
In approximate dynamical equations, inhomogenous classical (mean) gauge and Higgs fields are coupled to quantized fermions. The equations are solved numerically on a spacetime lattice. The fermions appear to equilibrate according to the Fermi-Dirac distribution with time-dependent temperature and chemical potential.
γµDµuα = 0, γµDµvα = 0.
Next define the fermion operator ψˆ,
ψˆ(x) = [ˆbαuα(x) + dˆ†αvα(x)],
α
in terms of annihilation and creation operators ˆbα, ˆb†α, . . . . The fermion back reaction is then specified by the initial conditions ˆb†αˆbα′ = nα δαα′ , dˆ†αdˆα′ = n¯α δαα′ , etc.
=
[1

Np(t)

N¯−p(t)]
p ωp(t)
,
Tr iγ0S(p, t) = 1 − Np(t) + N¯−p(t),
ωp(t) = m2p(t) + p2,
with Tr γ5S(p, t) = 0 because of parity invariance. For free fermions Np, N¯p and m are time-independent. Assuming that the interacting model can be described approximately by quasiparticles, we now use the above equations to define Np(t), N¯p(t) and mp(t). In a non-equilibrium situation they will depend on time.
[4] for local (in time) equilibration of fermions by comparing their distribution function with the Fermi-Dirac distribution. The distribution function was identified from the equal-time fermion two point function, averaged over space (a circle with circumference L),
where we have specialized to zero Yukawa coupling. The fermion backreaction is specified as follows. Introduce a complete set of orthonormal mode functions uα, vα for the fermions, which satisfy the Dirac equation
Fig. 1 shows the Chern-Simons number C = − dx A1/2π and the axial charge Q5 /nf for a simulation starting with a fermionic vacuum (i.e. nα, n¯α = 0) and some kinetic energy stored in a few low momentum modes of the Higgs field. The anomalous fermion number non-conservation equation ∆ Q5 = nf ∆C, is well obeyed since the two curves are indistinguishable (initially Q5 = C = 0). The oscillations correspond roughly to the basic period 2π/mA. To smoothen these we average S(p, t) over a time interval tav before extracting the distribution functions. We used etav = 4 and studied the behavior of Navp(t) ≡
porter U (x, y) = exp[−i
y xdzຫໍສະໝຸດ A1(z)/2].
We have
used the latter method, but it is actually closely
related to complete Coulomb gauge fixing [4]. If
the fermions were free, the Fourier transform
3. Here we are especially interested in thermalization properties of the fermions. We tested
2
C,〈Q5〉/nf log (1/Nav−1)
0.5
0.0
−0.5
−1.0
−1.5 0.0
10.0
20.0
30.0
40.0
50.0
et
Figure 1. Chern-Simons number C and axial charge Q5 /nf versus time in units 1/e.
et=2
10.0
et=18
et=34
7.5
5.0
2.5
0.0
−0.6
−0.4
−0.2
0.0
0.2
0.4
0.6
ap
Figure 2. Least squares straight line fits to ln(Na−v1p − 1) versus ap.
1
ITFA-99-23 THU-99-26
Real-time dynamics in the 1+1 D abelian Higgs model with fermions∗
Gert Aartsa and Jan Smitb,a
aInstitute for Theoretical Physics, Utrecht University Princetonplein 5, 3584 CC Utrecht, the Netherlands
The above system of equations has been implemented on a lattice using Wilson’s fermion method for the spatial derivative and the staggered fermion interpretation for a ‘naive’ discrete time derivative [3]. Usual expectations on fermion number non-conservation tied to sphaleron transitions are correctly represented on the lattice. For simplicity we continue with continuum notation.
S(z, t)
=
1 L
L
dx ψ(x, t)ψ¯(x + z, t) g.f..
0
Here g.f. indicates a complete gauge fixing. Alter-
natively, the two point function can be rendered
gauge invariant by supplying a parallel trans-
L
S(p, t) = dz e−ipz S(z, t)
0
would be given in terms of distribution functions Np, N¯p als follows:
Tr S(p, t)
=
[1

Np(t)

N¯−p(t)]
mp(t) ωp(t)
,
Tr iγ1S(p, t)
The simulations had the following parameters: nf = 2 flavors (related to fermion doubling in time), spatial size mϕL ≈ 6.4, λ/e2 = 0.25 (mAL ≈ 9), coupling e2/m2ϕ ≈ 0.25, with spatial lattice spacing amϕ ≈ 0.10, temporal spacing a0/a = 0.005 and L/a = 64 spatial lattice sites.
2. The 1+1 D abelian Higgs model coupled axially to fermions is qualitatively similar to the electroweak sector of the Standard Model. As for the SU(2) case in 4D, it can be rewritten in a form with vectorial gauge couplings and MajoranaYukawa couplings. For N → ∞ fermion replicas, the equations of motion reduce to a classical field approximation for the bosonic variables, with a
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