Where does the hot electroweak phase transition end

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《时光之光 - Hotcha 叶文辉》歌词 Hotcha

《时光之光 - Hotcha 叶文辉》歌词 Hotcha

时光之光- Hotcha 叶文辉
Hotcha&叶文辉- 时光之光
一宗宗瘟疫正在市内迅速蔓延吧
巴不得伸尽我的舌尖食了它
一帮帮幽灵正在市内暗中战斗吗
巴不得即刻交由我们去追杀
Woo o oh oh ( R ) 街里空气有些烟
Woo o oh o oh ( W ) 等你因我想大变
Woo o oh oh ( C ) 心里知觉有些黏Woo o oh o oh ( All ) 等我拉你走到时代前面
掴一巴大厦降雪花
乱放一枪围城脱野马
插一刀尽量要动作很大
嗌一声闷局会转弯
大吃一惊原来可变化
请跟我变得很伟大
一支支魔笛正在市内奏出未来吧
巴不得伸尽我的脚踭踏碎它
一堆堆乌云正在市内压低兴致吗
巴不得即刻交由我们去蒸发
Woo o oh oh ( R ) 街里空气有些烟
Woo o oh o oh ( W ) 等你因我想大变
Woo o oh oh ( C ) 心里知觉有些黏
Woo o oh o oh ( All ) 等我拉你走到时代前面
掴一巴大厦降雪花
乱放一枪围城脱野马
插一刀尽量要动作很大
嗌一声闷局会转弯
大吃一惊原来可变化
请跟我变得很伟大
要是太坏就要一巴掴它
要是太静就要嗌它
掴一巴大厦降雪花
乱放一枪围城脱野马
插一刀尽量要动作很大
嗌一声闷局会转弯
大吃一惊原来可变化
抑郁会变小当我姿势大
以上就是关于时光之光- Hotcha 叶文辉的歌词,感谢您的阅读!。

热场的重要性英语作文

热场的重要性英语作文

热场的重要性英语作文The Importance of Warm-Up in Any Event or Performance.The significance of warm-up extends far beyond a mere ritual or a routine exercise. It is an integral part of any event or performance, whether it's a sports match, a concert, or any other form of competition or exhibition.The warm-up phase serves multiple purposes, from psychological preparation to physiological readiness, ensuring that participants are at their peak when itmatters most.Psychological Preparation.Before any major event, the mind needs to be asprepared as the body. The warm-up is a time for athletes or performers to gather their thoughts, focus their energy,and visualize success. It's a transition period from the calm before the storm to the intense action that lies ahead. By going through familiar routines and movements, they canease their anxiety, build their confidence, and enter a state of flow where they are fully immersed in the task at hand.Physiological Readiness.Physiologically, the warm-up serves a crucial purposein preparing the body for the demands of the event. It raises the body temperature, increasing muscle elasticity and reducing the risk of injury. It also primes the cardiovascular system, getting the heart rate up and the blood flowing more efficiently, ensuring that oxygen and nutrients are delivered to the muscles more rapidly. This not only improves performance but also helps preventfatigue and cramps.Increasing Muscle Efficiency.The warm-up involves a gradual increase in intensity, allowing the muscles to gradually adapt and prepare for the rigors of the main event. This progressive warming up of the muscles helps to increase their efficiency, allowingthem to contract and relax more quickly and smoothly. This, in turn, leads to better control, more power, and less wasted energy.Improving Coordination and Balance.The warm-up routines often involve dynamic stretches and movements that improve coordination and balance. These exercises help athletes or performers to become more aware of their body's position and movement, enabling them to execute complex skills or maneuvers with greater precision and control.Preventing Injuries.One of the most overlooked benefits of the warm-up is its role in injury prevention. By gradually increasing the intensity of exercise, the warm-up helps to lubricate the joints, increase blood flow to the muscles, and prepare the ligaments and tendons for the stresses they will encounter during the main event. This conditioning effect can significantly reduce the risk of pulls, tears, or otheracute injuries.Enhancing Performance.Finally, the warm-up is a critical component of peak performance. By raising the body's temperature, increasing muscle efficiency, and improving coordination, the warm-up primes the body for optimal performance. Whether it's a runner's final strides before a race, a dancer's practice moves before a show, or a musician's scale runs before a concert, the warm-up is the invisible yet essential ingredient that can turn good performances into great ones.In conclusion, the warm-up is not just a routine exercise; it's a critical component of any event or performance. It serves to prepare both the mind and the body, ensuring that participants are ready to perform at their highest level when it counts. Whether it's a competitive edge or a personal best, the warm-up is often the key to unlocking one's full potential.。

河北省邢台市第二中学2021届高三英语上学期11月月考试题含解析

河北省邢台市第二中学2021届高三英语上学期11月月考试题含解析

某某省某某市第二中学2021届高三英语上学期11月月考试题(含解析)第一部分听力(共两节,满分30 分)第一节(共5 小题:每小题1. 5 分,满分7. 5 分)1.How will the man go home?A. By bike.B. By subway.C. By bus. 2.What happened to the woman’s son?A. He hurt his arm.B. He had a headache.C. He got pains in his fingers.3.What will the man do tonight?A. Do his homework.B. Watch TV.C. Play football. 4.What is Mary’s phone number?A. 97756431.B. 86727151.C. 86727115.5. What is the man looking for?A. A puter.B. A cup of tea.C. A book.第二节(共15 小题;每小题1. 5 分,满分22. 5 分)听第6 段材料,回答第6、7 题。

6. What will the woman do for Albert’s birthday?A. Decorate his room.B. Organize a party.C. Prepare a big dinner.7.What does the woman ask the man to bring?A. Juice.B. A cake.C. Fruit.听第7 段材料,回答第8、9 题8.What are the speakers mainly talking about?A. An interview.B. An English class.C.A piece of homework.9.What did Mr. Gray talk a lot about?A. The methods of learning English.B. The culture of some countries.C. The rules in the classroom.听第8 段材料,回答第10 至12 题。

the technicolor phase中英文歌词

the technicolor phase中英文歌词

I am the red in the rose, the flowers on the blankets on your bedroom floor And I am the gray in the ghostthat hides with your clothes behind your closet doorI am the green in the grass that bends back from underneath your feetAnd I am the blue in your back-alley view where the horizon and the rooftops meetIf you cut me I suppose I would bleed the colors of the evening starsYou can go anywhere you wish cuz I’ll be there, wherever you areI will always meet your gazeWhen we are lost in the Technicolor phaseI am the black in the book, the letters on the pages that you memorizeAnd I am the orange in the overcast, a color that you visualizeI am the white in the walls that soak up all the sound when you cannot sleep And I am the peach in the starfish on the beachthat wish the harbor wasn’t quite so deepmy darlingwherever you are~~我是玫瑰里的一点红晕是你闺中地毯上那丛花瓣我是被施了咒语的魔里的灰把自己藏在你的门后飘动的裙带我是你踏过后又追着你的气息不忍躺去的青草我是夕阳与那屋檐汇聚的地方你残留的涩伤你若真忍心伤我那我的血滴定能染红夜间所有的星我愿追你不离不弃到天际我愿追随你的目光当我们在城市的光怪陆离里迷失自己也许最初你的生命里没有我的位置,在你悄然发觉的那一页我是天边为你绚烂的火烧云,一种让你回眸的颜色当你辗转反侧难以入眠,我定然是那面墙壁,为你驱逐去所有世间吵杂我是与沙滩上海星嬉戏的阳光希望这巷儿没有这般悠长我的至爱无论你身处何方。

惠普彩色激光打印机 Pro M454 和惠普彩色激光多功能一体机 Pro M479 维修手册说明书

惠普彩色激光打印机 Pro M454 和惠普彩色激光多功能一体机 Pro M479 维修手册说明书

Table -1 Revision history Revision number 1
Revision date 6/2019
Revision notes HP LaserJet Pro M454 HP LaserJet Pro MFP M479 Repair manual initial release
Additional service and support for HP internal personnel HP internal personnel, go to one of the following Web-based Interactive Search Engine (WISE) sites: Americas (AMS) – https:///wise/home/ams-enWISE - English – https:///wise/home/ams-esWISE - Spanish – https:///wise/home/ams-ptWISE - Portuguese – https:///wise/home/ams-frWISE - French Asia Pacific / Japan (APJ) ○ https:///wise/home/apj-enWISE - English ○ https:///wise/home/apj-jaWISE - Japanese ○ https:///wise/home/apj-koWISE - Korean ○ https:///wise/home/apj-zh-HansWISE - Chinese (simplified)
Find information about the following topics ● Service manuals ● Service advisories ● Up-to-date control panel message (CPMD) troubleshooting ● Install and configure ● Printer specifications ● Solutions for printer issues and emerging issues ● Remove and replace part instructions and videos ● Warranty and regulatory information

《频域采样定理》课件

《频域采样定理》课件

结论
频域采样定理对信号处理具有重要意义,我们总结了它的重要性,也提出了 该领域未来的发展趋势。 此外,我们补充了相关领域的研究方法,为进一步深入研究提供了方向。
参考文献
• Nyquist,H.(1928)Thermal agitation of electric charge in conductors。Physical Review. 32(1):110–113 • Shannon,C. E. (1949). Communication in the presence of noise. Proceedings of the IRE, 37(1), 10-21.
采定理的推导
为了理解采样定理,首先需要了解采样的基本过程以及与频域采样定理的联 系。 我们将阐述采样定理的推导过程及相关公式,并详细讨论Nyquist采样定理。
应用
频域采样定理在通信领域中有着广泛的应用,它可以保证信号在传输过程中 不失真。
此外,频域采样定理也在音频与视频处理、DAC与ADC芯片的设计与应用中发 挥着重要作用。
《频域采样定理》PPT课 件
欢迎来到本次《频域采样定理》的PPT课件。本次课件将深入浅出地介绍频域 采样定理的概念、推导、应用及未来发展趋势。
什么是频域采样定理
频域采样定理是指在信号采样过程中,要使得信号能够完全还原,采样频率必须满足一定的条件。 这一定理与信号重构密切相关,我们将探讨其原理和应用。

PowerWeld Gouging Carbon产品安全数据表说明书

PowerWeld Gouging Carbon产品安全数据表说明书

S AFETY D ATA S HEETSection 1: Product and Company IdentificationProduct Identifier:PowerWeld Gouging CarbonsProduct Use:Arc Air GougingItem Code:DC__; DCF__; DCJ__Supplier Name:Techniweld CorporationSupplier Address:2300 Winston Park DriveOakville, ON L6H 7T7Supplier Web Address:Supplier Phone: 905-829-87801-800-268-4833Emergency Phone:CHEMTREC (800) 424-9300Prepared By:Techniweld CorporationPreparation Date:18 January 2016Section 2: Hazard IdentificationClassification:Not classifiedLabel Elements: See labelOther Hazards: Product is not hazardous as shipped, but may be hazardous during thegouging process: overexposure to fumes and gases may be detrimental tohealth; beware of spatter, hot metal and slag as this can burn skin and causefire; excessive noise is likely; arc rays can injure eyes and burn skin; electricshock can kill; avoid touching live electrical parts.Section 3: Composition/Information on Hazardous IngredientsHAZARDOUS INGREDIENTS CAS NUMBERAPPROXIMATE CONCENTRATION (%)Fixed Carbon [graphite] (C) 7440-44-0 [7782-42-5]>95Copper (Cu) 7440-50-8 <5Section 4: First-aid MeasuresInhalation:Inhalation may be the most common cause of overexposure due to thefumes. Large amounts of fumes will cause irritation of the nose, eyes andskin. Move from the area that has any fumes to fresh air. If breathing isdifficult, give oxygen. If not breathing, give artificial respiration andtransport to nearest medical facility for additional treatment.Ingestion:Not an expected route of exposure. Rinse month completely and drink a cupof water if conscious; obtain medical assistance when needed.Eye Contact:If arc flash or burns occur, obtain medical assistance. Large exposure towelding fumes may cause irritation to the eyes. Immediately flush upperand lower eyelids with plenty of water. After initial flushing, remove anycontact lenses and continue flushing for at least 15 minutes. Rest eyes for30 minutes. If redness, burning, blurred vision or swelling persists, visitnearest medical facility for additional treatment.8728990Skin Contact:Large exposure to welding fumes may cause irritation to skin. If burnsoccur, flush with clean cool water for 15 minutes; obtain medical assistancewhen needed.NOTE: In all severe cases, contact physician immediately. Local telephone operators can provide number of regional poison control centre.Section 5: Fire-fighting MeasuresFlammable:NoMeans of Extinction:Not applicableAuto-ignition Temperature:Not applicableHazardous Combustion Products: Not applicableExplosion Data Sensitivity toMechanical Impact:Not applicableExplosion Data Sensitivity toStatic Discharge: Not applicableSpecial Equipment:This product as shipped is non-flammable; however, gouging should nottake place in the presence of flammable materials, vapours, tanks, pipes, orcontainers that have held flammable substances unless otherwise certifiedas safe.Precautions for Fire Fighters:Firefighters should wear proper protective equipment and self-containedbreathing apparatus with full face piece. Shield personnel to protect fromventing, rupturing or bursting cans. Move containers from fire area if it canbe done without risk. Water spray may be useful in cooling equipment andcans exposed to heat and flame.Section 6: Accidental Release MeasuresProtective Equipment:See section 8Emergency Procedures:Product as shipped has no hazards.Leak or Spill Procedure:Product can be swept and removed, remaining alert to the possibility of hotends if recently used in the gouging process.Section 7: Handling and StorageHandling Procedures and Equipment:No special equipment is required to handle product as shipped. Handle inaccordance with good industrial hygiene and safety practices. Do not eat,drink or smoke when using this product. Wash hands thoroughly beforebreaks and at the end of the workday.Storage Requirements:Store in a cool, dry and low humid location as moist electrodes may shatterviolently if used (dry moist electrodes by baking at 300°F for 10 hours).Incompatibilities:None knownSection 8: Exposure Controls/Personal ProtectionExposure Limits:HAZARDS CAS NUMBER TLV-TWACopper (Cu) 7440-50-8 0.2 mg/m3 (fume), 1.0 mg/m3 (dust)Graphite 7440-44-0 2 mg/m3 (resp)Carbon Dioxide (CO2) 124-38-9 5000 ppmCarbon Monoxide (CO) 630-08-0 25 ppmNitrogen Dioxide (NO2) 10102-44-0 0.2 ppmOzone (O3) 10028-15-6 -Nitrogen Monoxide (NO) 10102-43-9 25 ppmEngineering Controls:General ventilation and local fume extraction must be adequate to keepfume concentrations within safe limits; respiratory protection should beused during the arc gouging process. Arcs and sparks during arc gougingcan be source of ignition of combustible materials. Take precautions toprevent fires.Personal Protective Equipment:Respiratory: A properly fitting fume respirator or air supplied respiratorshould be used where local exhaust and/or ventilation does not keepexposure below threshold limits indicated above.Hands: For use during the arc gouging process, properly fitted and certifiedgloves (ie./ leather welding gloves) are recommended to prevent injuryfrom sparks and electric shock.Eyes: An approved welding helmet or face shield with a filter lens shade 12-14 or higher is recommended. Other persons around the workspace shouldalso be protected by shaded welding screens and eyewear if necessary.Skin: Approved protection (ie./ welders gloves, apron, sleeves, jacket, etc.)should be worn to prevent injury from sparks and electrical shock. Section 9: Physical and Chemical PropertiesPhysical State:Solid (stick/bar)Odour and Appearance:Odourless copper coloured rod with black tipsOdour Threshold (ppm): Not applicablepH: Not applicableMelting Point:Not applicableFreezing Point: Not applicableBoiling Point:Not applicableFlashpoint:Not applicableUpper Flammable Limit (% by volume):Not applicableLower Flammable Limit (% by volume):Not applicableSection 10: Stability and ReactivityChemical Stability:StablePossible Hazardous Reactions:None knownConditions to Avoid:None under normal conditionsMaterials to Avoid (Incompatibilities):None knownConditions of Reactivity:Not availableHazardous Decomposition By-Products: When burning – CO2, CO and traces of copper fumes (Ozone, Nitrogen Oxidefrom electric and UV rays)Section 11: Toxicological InformationSkin Contact:Arc rays can burn skin; skin cancer has been reported.Skin Absorption: Not applicableEye Contact:Arc rays can injure eyes.Inhalation:Inhalation is the most likely route of exposure; refer to “Effects of AcuteExposure” and “Effects of Chronic Exposure” below.Ingestion:Unlikely due to the form of product.Effects of Acute Exposure:Radiant energy can produce flash burns of eyes and skin. Electric shock cankill. Over exposure to fumes can cause personal injury. Symptoms can varyaccording to gouging process. These may include breathing difficulty,headache, nausea, dryness or irritation of nose, throat, eyes, burningsensation of skin or eyes, unconsciousness.Effects of Chronic Exposure:Overexposure or prolonged inhalation may cause bronchitis, lung depositsand tissue damage which may be irreversible. Exposure to ultra-violet arcrays can result in keratosis-conjunctivitis causing inflammation, blurredvision, headache, sunburn.Irritancy of Product:Not availableSensitization to Product:May cause sensitisation by skin contact.Carcinogenicity:Welding fumes may be carcinogenic to humans.Reproductive Effects:Not availableToxicological Data:Not availableSection 12: Ecological InformationAquatic and Terrestrial Toxicity:The welding process can affect the environment if fume is released directlyinto the atmosphere. Residues from welding consumables could degradeand accumulate into soils and ground water.Acute fish toxicityLC50 Fish 96h Manganese: 2.91 mg/lAluminum oxide: >100 mg/l Salmo truttaLC50 Algae 72h Manganese: 0.55 mg/lAluminum oxide: >100 mg/l Selenastrumcapricornatum (greenalgae)EC50 Daphnia 48h Manganese: 5.2 mg/lAluminum oxide: >100 mg/l Daphina magna(Water flea) Persistence and Degradability:Not availableBioaccumulative Potential:Bio concentration factor (BCF): Iron 140 000Manganese 59052 Soil Mobility:Not availableSection 13: Disposal ConsiderationsNOTE: Always dispose of waste in accordance with local, provincial and federal regulations.Safe Handling:Gloves can be worn when handling used and discarded materials. Product isnot harmful as shipped.Methods of Disposal:Avoid dispersal and contact of spilled material and runoff with soil,waterways, drains and sewers. Packaging and tungsten electrode stubs canbe disposed of as general waste or recycled. For larger quantities, be sure todispose in accordance with local, provincial/state and federal regulations. Section 14: Transportation InformationAs finished product, gouging carbons are not subject to special shipping conditions.Section 15: Regulatory InformationCanada WHMIS Classification:Class D; Division 2, Subdivision ACanadian Environmental ProtectionAct (CEPA):All constituents of these products are on the Domestic Substance List (DSL).California Proposition 65:These products contain or produce chemicals known to the State ofCalifornia to cause cancer, birth defects or other reproductive harm.United States Toxic SubstancesControl Act (TSCA): All constituents of these products are on the TSCA inventory list orexcluded from listing.Section 16: Other InformationPreparation Date:18 January 2016Date of Last Revision:18 January 2016This SDS format is in accordance with GHS. Techniweld Corporation provides the information contained herein in good faith but makes no representation as to its comprehensiveness or accuracy. This document is intended only as a guide to the appropriate precautionary handling of the material by a properly trained person using this product. Product use and conditions of use are beyond the control of Techniweld. Warranty of materials is limited to test results of product performance as detailed in certificates of compliance. Interpretation of test results is the responsibility of end-user. No other warranties, expressed or implied, are made.。

物理学专业英语

物理学专业英语

华中师范大学物理学院物理学专业英语仅供内部学习参考!2014一、课程的任务和教学目的通过学习《物理学专业英语》,学生将掌握物理学领域使用频率较高的专业词汇和表达方法,进而具备基本的阅读理解物理学专业文献的能力。

通过分析《物理学专业英语》课程教材中的范文,学生还将从英语角度理解物理学中个学科的研究内容和主要思想,提高学生的专业英语能力和了解物理学研究前沿的能力。

培养专业英语阅读能力,了解科技英语的特点,提高专业外语的阅读质量和阅读速度;掌握一定量的本专业英文词汇,基本达到能够独立完成一般性本专业外文资料的阅读;达到一定的笔译水平。

要求译文通顺、准确和专业化。

要求译文通顺、准确和专业化。

二、课程内容课程内容包括以下章节:物理学、经典力学、热力学、电磁学、光学、原子物理、统计力学、量子力学和狭义相对论三、基本要求1.充分利用课内时间保证充足的阅读量(约1200~1500词/学时),要求正确理解原文。

2.泛读适量课外相关英文读物,要求基本理解原文主要内容。

3.掌握基本专业词汇(不少于200词)。

4.应具有流利阅读、翻译及赏析专业英语文献,并能简单地进行写作的能力。

四、参考书目录1 Physics 物理学 (1)Introduction to physics (1)Classical and modern physics (2)Research fields (4)V ocabulary (7)2 Classical mechanics 经典力学 (10)Introduction (10)Description of classical mechanics (10)Momentum and collisions (14)Angular momentum (15)V ocabulary (16)3 Thermodynamics 热力学 (18)Introduction (18)Laws of thermodynamics (21)System models (22)Thermodynamic processes (27)Scope of thermodynamics (29)V ocabulary (30)4 Electromagnetism 电磁学 (33)Introduction (33)Electrostatics (33)Magnetostatics (35)Electromagnetic induction (40)V ocabulary (43)5 Optics 光学 (45)Introduction (45)Geometrical optics (45)Physical optics (47)Polarization (50)V ocabulary (51)6 Atomic physics 原子物理 (52)Introduction (52)Electronic configuration (52)Excitation and ionization (56)V ocabulary (59)7 Statistical mechanics 统计力学 (60)Overview (60)Fundamentals (60)Statistical ensembles (63)V ocabulary (65)8 Quantum mechanics 量子力学 (67)Introduction (67)Mathematical formulations (68)Quantization (71)Wave-particle duality (72)Quantum entanglement (75)V ocabulary (77)9 Special relativity 狭义相对论 (79)Introduction (79)Relativity of simultaneity (80)Lorentz transformations (80)Time dilation and length contraction (81)Mass-energy equivalence (82)Relativistic energy-momentum relation (86)V ocabulary (89)正文标记说明:蓝色Arial字体(例如energy):已知的专业词汇蓝色Arial字体加下划线(例如electromagnetism):新学的专业词汇黑色Times New Roman字体加下划线(例如postulate):新学的普通词汇1 Physics 物理学1 Physics 物理学Introduction to physicsPhysics is a part of natural philosophy and a natural science that involves the study of matter and its motion through space and time, along with related concepts such as energy and force. More broadly, it is the general analysis of nature, conducted in order to understand how the universe behaves.Physics is one of the oldest academic disciplines, perhaps the oldest through its inclusion of astronomy. Over the last two millennia, physics was a part of natural philosophy along with chemistry, certain branches of mathematics, and biology, but during the Scientific Revolution in the 17th century, the natural sciences emerged as unique research programs in their own right. Physics intersects with many interdisciplinary areas of research, such as biophysics and quantum chemistry,and the boundaries of physics are not rigidly defined. New ideas in physics often explain the fundamental mechanisms of other sciences, while opening new avenues of research in areas such as mathematics and philosophy.Physics also makes significant contributions through advances in new technologies that arise from theoretical breakthroughs. For example, advances in the understanding of electromagnetism or nuclear physics led directly to the development of new products which have dramatically transformed modern-day society, such as television, computers, domestic appliances, and nuclear weapons; advances in thermodynamics led to the development of industrialization; and advances in mechanics inspired the development of calculus.Core theoriesThough physics deals with a wide variety of systems, certain theories are used by all physicists. Each of these theories were experimentally tested numerous times and found correct as an approximation of nature (within a certain domain of validity).For instance, the theory of classical mechanics accurately describes the motion of objects, provided they are much larger than atoms and moving at much less than the speed of light. These theories continue to be areas of active research, and a remarkable aspect of classical mechanics known as chaos was discovered in the 20th century, three centuries after the original formulation of classical mechanics by Isaac Newton (1642–1727) 【艾萨克·牛顿】.University PhysicsThese central theories are important tools for research into more specialized topics, and any physicist, regardless of his or her specialization, is expected to be literate in them. These include classical mechanics, quantum mechanics, thermodynamics and statistical mechanics, electromagnetism, and special relativity.Classical and modern physicsClassical mechanicsClassical physics includes the traditional branches and topics that were recognized and well-developed before the beginning of the 20th century—classical mechanics, acoustics, optics, thermodynamics, and electromagnetism.Classical mechanics is concerned with bodies acted on by forces and bodies in motion and may be divided into statics (study of the forces on a body or bodies at rest), kinematics (study of motion without regard to its causes), and dynamics (study of motion and the forces that affect it); mechanics may also be divided into solid mechanics and fluid mechanics (known together as continuum mechanics), the latter including such branches as hydrostatics, hydrodynamics, aerodynamics, and pneumatics.Acoustics is the study of how sound is produced, controlled, transmitted and received. Important modern branches of acoustics include ultrasonics, the study of sound waves of very high frequency beyond the range of human hearing; bioacoustics the physics of animal calls and hearing, and electroacoustics, the manipulation of audible sound waves using electronics.Optics, the study of light, is concerned not only with visible light but also with infrared and ultraviolet radiation, which exhibit all of the phenomena of visible light except visibility, e.g., reflection, refraction, interference, diffraction, dispersion, and polarization of light.Heat is a form of energy, the internal energy possessed by the particles of which a substance is composed; thermodynamics deals with the relationships between heat and other forms of energy.Electricity and magnetism have been studied as a single branch of physics since the intimate connection between them was discovered in the early 19th century; an electric current gives rise to a magnetic field and a changing magnetic field induces an electric current. Electrostatics deals with electric charges at rest, electrodynamics with moving charges, and magnetostatics with magnetic poles at rest.Modern PhysicsClassical physics is generally concerned with matter and energy on the normal scale of1 Physics 物理学observation, while much of modern physics is concerned with the behavior of matter and energy under extreme conditions or on the very large or very small scale.For example, atomic and nuclear physics studies matter on the smallest scale at which chemical elements can be identified.The physics of elementary particles is on an even smaller scale, as it is concerned with the most basic units of matter; this branch of physics is also known as high-energy physics because of the extremely high energies necessary to produce many types of particles in large particle accelerators. On this scale, ordinary, commonsense notions of space, time, matter, and energy are no longer valid.The two chief theories of modern physics present a different picture of the concepts of space, time, and matter from that presented by classical physics.Quantum theory is concerned with the discrete, rather than continuous, nature of many phenomena at the atomic and subatomic level, and with the complementary aspects of particles and waves in the description of such phenomena.The theory of relativity is concerned with the description of phenomena that take place in a frame of reference that is in motion with respect to an observer; the special theory of relativity is concerned with relative uniform motion in a straight line and the general theory of relativity with accelerated motion and its connection with gravitation.Both quantum theory and the theory of relativity find applications in all areas of modern physics.Difference between classical and modern physicsWhile physics aims to discover universal laws, its theories lie in explicit domains of applicability. Loosely speaking, the laws of classical physics accurately describe systems whose important length scales are greater than the atomic scale and whose motions are much slower than the speed of light. Outside of this domain, observations do not match their predictions.Albert Einstein【阿尔伯特·爱因斯坦】contributed the framework of special relativity, which replaced notions of absolute time and space with space-time and allowed an accurate description of systems whose components have speeds approaching the speed of light.Max Planck【普朗克】, Erwin Schrödinger【薛定谔】, and others introduced quantum mechanics, a probabilistic notion of particles and interactions that allowed an accurate description of atomic and subatomic scales.Later, quantum field theory unified quantum mechanics and special relativity.General relativity allowed for a dynamical, curved space-time, with which highly massiveUniversity Physicssystems and the large-scale structure of the universe can be well-described. General relativity has not yet been unified with the other fundamental descriptions; several candidate theories of quantum gravity are being developed.Research fieldsContemporary research in physics can be broadly divided into condensed matter physics; atomic, molecular, and optical physics; particle physics; astrophysics; geophysics and biophysics. Some physics departments also support research in Physics education.Since the 20th century, the individual fields of physics have become increasingly specialized, and today most physicists work in a single field for their entire careers. "Universalists" such as Albert Einstein (1879–1955) and Lev Landau (1908–1968)【列夫·朗道】, who worked in multiple fields of physics, are now very rare.Condensed matter physicsCondensed matter physics is the field of physics that deals with the macroscopic physical properties of matter. In particular, it is concerned with the "condensed" phases that appear whenever the number of particles in a system is extremely large and the interactions between them are strong.The most familiar examples of condensed phases are solids and liquids, which arise from the bonding by way of the electromagnetic force between atoms. More exotic condensed phases include the super-fluid and the Bose–Einstein condensate found in certain atomic systems at very low temperature, the superconducting phase exhibited by conduction electrons in certain materials,and the ferromagnetic and antiferromagnetic phases of spins on atomic lattices.Condensed matter physics is by far the largest field of contemporary physics.Historically, condensed matter physics grew out of solid-state physics, which is now considered one of its main subfields. The term condensed matter physics was apparently coined by Philip Anderson when he renamed his research group—previously solid-state theory—in 1967. In 1978, the Division of Solid State Physics of the American Physical Society was renamed as the Division of Condensed Matter Physics.Condensed matter physics has a large overlap with chemistry, materials science, nanotechnology and engineering.Atomic, molecular and optical physicsAtomic, molecular, and optical physics (AMO) is the study of matter–matter and light–matter interactions on the scale of single atoms and molecules.1 Physics 物理学The three areas are grouped together because of their interrelationships, the similarity of methods used, and the commonality of the energy scales that are relevant. All three areas include both classical, semi-classical and quantum treatments; they can treat their subject from a microscopic view (in contrast to a macroscopic view).Atomic physics studies the electron shells of atoms. Current research focuses on activities in quantum control, cooling and trapping of atoms and ions, low-temperature collision dynamics and the effects of electron correlation on structure and dynamics. Atomic physics is influenced by the nucleus (see, e.g., hyperfine splitting), but intra-nuclear phenomena such as fission and fusion are considered part of high-energy physics.Molecular physics focuses on multi-atomic structures and their internal and external interactions with matter and light.Optical physics is distinct from optics in that it tends to focus not on the control of classical light fields by macroscopic objects, but on the fundamental properties of optical fields and their interactions with matter in the microscopic realm.High-energy physics (particle physics) and nuclear physicsParticle physics is the study of the elementary constituents of matter and energy, and the interactions between them.In addition, particle physicists design and develop the high energy accelerators,detectors, and computer programs necessary for this research. The field is also called "high-energy physics" because many elementary particles do not occur naturally, but are created only during high-energy collisions of other particles.Currently, the interactions of elementary particles and fields are described by the Standard Model.●The model accounts for the 12 known particles of matter (quarks and leptons) thatinteract via the strong, weak, and electromagnetic fundamental forces.●Dynamics are described in terms of matter particles exchanging gauge bosons (gluons,W and Z bosons, and photons, respectively).●The Standard Model also predicts a particle known as the Higgs boson. In July 2012CERN, the European laboratory for particle physics, announced the detection of a particle consistent with the Higgs boson.Nuclear Physics is the field of physics that studies the constituents and interactions of atomic nuclei. The most commonly known applications of nuclear physics are nuclear power generation and nuclear weapons technology, but the research has provided application in many fields, including those in nuclear medicine and magnetic resonance imaging, ion implantation in materials engineering, and radiocarbon dating in geology and archaeology.University PhysicsAstrophysics and Physical CosmologyAstrophysics and astronomy are the application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. Because astrophysics is a broad subject, astrophysicists typically apply many disciplines of physics, including mechanics, electromagnetism, statistical mechanics, thermodynamics, quantum mechanics, relativity, nuclear and particle physics, and atomic and molecular physics.The discovery by Karl Jansky in 1931 that radio signals were emitted by celestial bodies initiated the science of radio astronomy. Most recently, the frontiers of astronomy have been expanded by space exploration. Perturbations and interference from the earth's atmosphere make space-based observations necessary for infrared, ultraviolet, gamma-ray, and X-ray astronomy.Physical cosmology is the study of the formation and evolution of the universe on its largest scales. Albert Einstein's theory of relativity plays a central role in all modern cosmological theories. In the early 20th century, Hubble's discovery that the universe was expanding, as shown by the Hubble diagram, prompted rival explanations known as the steady state universe and the Big Bang.The Big Bang was confirmed by the success of Big Bang nucleo-synthesis and the discovery of the cosmic microwave background in 1964. The Big Bang model rests on two theoretical pillars: Albert Einstein's general relativity and the cosmological principle (On a sufficiently large scale, the properties of the Universe are the same for all observers). Cosmologists have recently established the ΛCDM model (the standard model of Big Bang cosmology) of the evolution of the universe, which includes cosmic inflation, dark energy and dark matter.Current research frontiersIn condensed matter physics, an important unsolved theoretical problem is that of high-temperature superconductivity. Many condensed matter experiments are aiming to fabricate workable spintronics and quantum computers.In particle physics, the first pieces of experimental evidence for physics beyond the Standard Model have begun to appear. Foremost among these are indications that neutrinos have non-zero mass. These experimental results appear to have solved the long-standing solar neutrino problem, and the physics of massive neutrinos remains an area of active theoretical and experimental research. Particle accelerators have begun probing energy scales in the TeV range, in which experimentalists are hoping to find evidence for the super-symmetric particles, after discovery of the Higgs boson.Theoretical attempts to unify quantum mechanics and general relativity into a single theory1 Physics 物理学of quantum gravity, a program ongoing for over half a century, have not yet been decisively resolved. The current leading candidates are M-theory, superstring theory and loop quantum gravity.Many astronomical and cosmological phenomena have yet to be satisfactorily explained, including the existence of ultra-high energy cosmic rays, the baryon asymmetry, the acceleration of the universe and the anomalous rotation rates of galaxies.Although much progress has been made in high-energy, quantum, and astronomical physics, many everyday phenomena involving complexity, chaos, or turbulence are still poorly understood. Complex problems that seem like they could be solved by a clever application of dynamics and mechanics remain unsolved; examples include the formation of sand-piles, nodes in trickling water, the shape of water droplets, mechanisms of surface tension catastrophes, and self-sorting in shaken heterogeneous collections.These complex phenomena have received growing attention since the 1970s for several reasons, including the availability of modern mathematical methods and computers, which enabled complex systems to be modeled in new ways. Complex physics has become part of increasingly interdisciplinary research, as exemplified by the study of turbulence in aerodynamics and the observation of pattern formation in biological systems.Vocabulary★natural science 自然科学academic disciplines 学科astronomy 天文学in their own right 凭他们本身的实力intersects相交,交叉interdisciplinary交叉学科的,跨学科的★quantum 量子的theoretical breakthroughs 理论突破★electromagnetism 电磁学dramatically显著地★thermodynamics热力学★calculus微积分validity★classical mechanics 经典力学chaos 混沌literate 学者★quantum mechanics量子力学★thermodynamics and statistical mechanics热力学与统计物理★special relativity狭义相对论is concerned with 关注,讨论,考虑acoustics 声学★optics 光学statics静力学at rest 静息kinematics运动学★dynamics动力学ultrasonics超声学manipulation 操作,处理,使用University Physicsinfrared红外ultraviolet紫外radiation辐射reflection 反射refraction 折射★interference 干涉★diffraction 衍射dispersion散射★polarization 极化,偏振internal energy 内能Electricity电性Magnetism 磁性intimate 亲密的induces 诱导,感应scale尺度★elementary particles基本粒子★high-energy physics 高能物理particle accelerators 粒子加速器valid 有效的,正当的★discrete离散的continuous 连续的complementary 互补的★frame of reference 参照系★the special theory of relativity 狭义相对论★general theory of relativity 广义相对论gravitation 重力,万有引力explicit 详细的,清楚的★quantum field theory 量子场论★condensed matter physics凝聚态物理astrophysics天体物理geophysics地球物理Universalist博学多才者★Macroscopic宏观Exotic奇异的★Superconducting 超导Ferromagnetic铁磁质Antiferromagnetic 反铁磁质★Spin自旋Lattice 晶格,点阵,网格★Society社会,学会★microscopic微观的hyperfine splitting超精细分裂fission分裂,裂变fusion熔合,聚变constituents成分,组分accelerators加速器detectors 检测器★quarks夸克lepton 轻子gauge bosons规范玻色子gluons胶子★Higgs boson希格斯玻色子CERN欧洲核子研究中心★Magnetic Resonance Imaging磁共振成像,核磁共振ion implantation 离子注入radiocarbon dating放射性碳年代测定法geology地质学archaeology考古学stellar 恒星cosmology宇宙论celestial bodies 天体Hubble diagram 哈勃图Rival竞争的★Big Bang大爆炸nucleo-synthesis核聚合,核合成pillar支柱cosmological principle宇宙学原理ΛCDM modelΛ-冷暗物质模型cosmic inflation宇宙膨胀1 Physics 物理学fabricate制造,建造spintronics自旋电子元件,自旋电子学★neutrinos 中微子superstring 超弦baryon重子turbulence湍流,扰动,骚动catastrophes突变,灾变,灾难heterogeneous collections异质性集合pattern formation模式形成University Physics2 Classical mechanics 经典力学IntroductionIn physics, classical mechanics is one of the two major sub-fields of mechanics, which is concerned with the set of physical laws describing the motion of bodies under the action of a system of forces. The study of the motion of bodies is an ancient one, making classical mechanics one of the oldest and largest subjects in science, engineering and technology.Classical mechanics describes the motion of macroscopic objects, from projectiles to parts of machinery, as well as astronomical objects, such as spacecraft, planets, stars, and galaxies. Besides this, many specializations within the subject deal with gases, liquids, solids, and other specific sub-topics.Classical mechanics provides extremely accurate results as long as the domain of study is restricted to large objects and the speeds involved do not approach the speed of light. When the objects being dealt with become sufficiently small, it becomes necessary to introduce the other major sub-field of mechanics, quantum mechanics, which reconciles the macroscopic laws of physics with the atomic nature of matter and handles the wave–particle duality of atoms and molecules. In the case of high velocity objects approaching the speed of light, classical mechanics is enhanced by special relativity. General relativity unifies special relativity with Newton's law of universal gravitation, allowing physicists to handle gravitation at a deeper level.The initial stage in the development of classical mechanics is often referred to as Newtonian mechanics, and is associated with the physical concepts employed by and the mathematical methods invented by Newton himself, in parallel with Leibniz【莱布尼兹】, and others.Later, more abstract and general methods were developed, leading to reformulations of classical mechanics known as Lagrangian mechanics and Hamiltonian mechanics. These advances were largely made in the 18th and 19th centuries, and they extend substantially beyond Newton's work, particularly through their use of analytical mechanics. Ultimately, the mathematics developed for these were central to the creation of quantum mechanics.Description of classical mechanicsThe following introduces the basic concepts of classical mechanics. For simplicity, it often2 Classical mechanics 经典力学models real-world objects as point particles, objects with negligible size. The motion of a point particle is characterized by a small number of parameters: its position, mass, and the forces applied to it.In reality, the kind of objects that classical mechanics can describe always have a non-zero size. (The physics of very small particles, such as the electron, is more accurately described by quantum mechanics). Objects with non-zero size have more complicated behavior than hypothetical point particles, because of the additional degrees of freedom—for example, a baseball can spin while it is moving. However, the results for point particles can be used to study such objects by treating them as composite objects, made up of a large number of interacting point particles. The center of mass of a composite object behaves like a point particle.Classical mechanics uses common-sense notions of how matter and forces exist and interact. It assumes that matter and energy have definite, knowable attributes such as where an object is in space and its speed. It also assumes that objects may be directly influenced only by their immediate surroundings, known as the principle of locality.In quantum mechanics objects may have unknowable position or velocity, or instantaneously interact with other objects at a distance.Position and its derivativesThe position of a point particle is defined with respect to an arbitrary fixed reference point, O, in space, usually accompanied by a coordinate system, with the reference point located at the origin of the coordinate system. It is defined as the vector r from O to the particle.In general, the point particle need not be stationary relative to O, so r is a function of t, the time elapsed since an arbitrary initial time.In pre-Einstein relativity (known as Galilean relativity), time is considered an absolute, i.e., the time interval between any given pair of events is the same for all observers. In addition to relying on absolute time, classical mechanics assumes Euclidean geometry for the structure of space.Velocity and speedThe velocity, or the rate of change of position with time, is defined as the derivative of the position with respect to time. In classical mechanics, velocities are directly additive and subtractive as vector quantities; they must be dealt with using vector analysis.When both objects are moving in the same direction, the difference can be given in terms of speed only by ignoring direction.University PhysicsAccelerationThe acceleration , or rate of change of velocity, is the derivative of the velocity with respect to time (the second derivative of the position with respect to time).Acceleration can arise from a change with time of the magnitude of the velocity or of the direction of the velocity or both . If only the magnitude v of the velocity decreases, this is sometimes referred to as deceleration , but generally any change in the velocity with time, including deceleration, is simply referred to as acceleration.Inertial frames of referenceWhile the position and velocity and acceleration of a particle can be referred to any observer in any state of motion, classical mechanics assumes the existence of a special family of reference frames in terms of which the mechanical laws of nature take a comparatively simple form. These special reference frames are called inertial frames .An inertial frame is such that when an object without any force interactions (an idealized situation) is viewed from it, it appears either to be at rest or in a state of uniform motion in a straight line. This is the fundamental definition of an inertial frame. They are characterized by the requirement that all forces entering the observer's physical laws originate in identifiable sources (charges, gravitational bodies, and so forth).A non-inertial reference frame is one accelerating with respect to an inertial one, and in such a non-inertial frame a particle is subject to acceleration by fictitious forces that enter the equations of motion solely as a result of its accelerated motion, and do not originate in identifiable sources. These fictitious forces are in addition to the real forces recognized in an inertial frame.A key concept of inertial frames is the method for identifying them. For practical purposes, reference frames that are un-accelerated with respect to the distant stars are regarded as good approximations to inertial frames.Forces; Newton's second lawNewton was the first to mathematically express the relationship between force and momentum . Some physicists interpret Newton's second law of motion as a definition of force and mass, while others consider it a fundamental postulate, a law of nature. Either interpretation has the same mathematical consequences, historically known as "Newton's Second Law":a m t v m t p F ===d )(d d dThe quantity m v is called the (canonical ) momentum . The net force on a particle is thus equal to rate of change of momentum of the particle with time.So long as the force acting on a particle is known, Newton's second law is sufficient to。

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a r X i v :h e p -p h /9809293v 2 15 S e p 19981ITP-Budapest 545Where does the hot electroweak phase transition end?F.Csikor,Z.Fodoraand J.Heitgerb ∗a Institute for Theoretical Physics,E¨o tv¨o s University,H-1088Budapest,Hungary bInstitut f¨u r Theoretische Physik I,Universit¨a t M¨u nster,D-48149M¨u nster,GermanyWe give the nonperturbative phase diagram of the four-dimensional hot electroweak phase transition.A sys-tematic extrapolation a →0is done.Our results show that the finite temperature SU(2)-Higgs phase transition is of first order for Higgs-boson masses m H <66.5±1.4GeV.The full four-dimensional result agrees completely with that of the dimensional reduction approximation.This fact is of particular importance,because it indicates that the fermionic sector of the Standard Model (SM)can be included perturbatively.We obtain that the Higgs-boson endpoint mass in the SM is 72.4±1.7GeV.Taking into account the LEP Higgs-boson mass lower bound excludes any electroweak phase transition in the SM.The observed baryon asymmetry is finally de-termined at the electroweak phase transition (EWPT)[1].The perturbative approach breaks down for the physically allowed Higgs-boson masses (e.g.m H >70GeV)[2].Since merely the bosonic sector is responsible for the bad perturba-tive features (due to infrared problems)the simu-lations are done without the inclusion of fermions on four-dimensional lattices [3],[4].Another ap-proach is the simulations of the reduced model in three-dimensions [5],[6].The comparison of the results obtained by the two techniques is not only a useful cross-check on the perturbative re-duction procedure but also a necessity because the fermions must be included perturbatively.The line separating the symmetric and broken phases on the m H −T c plane has an endpoint,m H,c .In four dimension at m H ≈80GeV the EWPT turned out to be extremely weak,even consistent with the no phase transition scenario on the 1.5-σlevel [7].Three-dimensional results show that for m H >95GeV no first order phase transition exists [8]and more specifically that the endpoint is m H,c ≈67GeV [9].In this paper we present the analysis of the endpoint on four dimensional lattices in the continuum limit and transform the result to the full SM.We will use different spacings in temporal (a t )and spatial (a s )directions.The asymmetry of the lattice spacings is given by the asymmetry factor2Tr U pl+βttp1−12Tr (ϕ+x ϕx )+λ12of bare parameters.The position on the LCP gives the lattice spacing a.As the lattice spacing decreases R HW,c→R HW,cont..Since our theory is a bosonic one we assumed that the corrections are quadratic in the latticespacings;thus an a2fit has been performed for R HW,c to determine its continuum value.We have carried out T=0simulations on L t=2,3,4,5lattices and tunedκto the tran-sition point.This conditionfixes the lattice spac-ings:a t=a s/ξ=1/(T c L t)in terms of the tran-sition temperature T c in physical units.The third parameterλ,finally specifying the physical Higgs mass in lattice units,has been chosen in a way that the transition corresponds to the endpoint of thefirst order phase transition subspace.In this paper V=L t·L3s type four-dimensional lattices are used.For each L t we had8different lattices,each of them had approximately twice as large lattice-volume as the previous one.The smallest lattice was V=2·53and the largest one was V=5·503.Reweighting was used to obtain information in the vicinity of a simulation point. The determination of the endpoint of thefinite temperature EWPT is done by the useof the Lee-Yang zeros of the partition function Z[12].Near thefirst order phase transition point the parti-tion function reads Z=Z s+Z b∝exp(−V f s)+ exp(−V f b),where the indices s(b)refer to the symmetric(broken)phase and f stands for the free-energy densities.Near the phase transition point we also have f b=f s+α(κ−κc),which shows that for complexκvalues Z vanishes at Im(κ)=π·(n−1/2)/(Vα)for integer n.In case afirst order phase transition is present,these Lee-Yang zeros move to the real axis as the volume goes to infinity.In case a phase transition is ab-sent the Lee-Yang zeros stay away from the real κaxis.Denotingκ0the lowest zero of Z,i.e. the position of the zero closest zero to the real axis,one expects in the vicinity of the endpoint the scaling law Im(κ0)=c1(L t,λ)Vν+c2(L t,λ). In order to pin down the endpoint we are look-ing for aλvalue for which c2vanish.In practice we analytically continue Z to complex values of κby reweighting the available data.Also small changes inλhave been done by reweighting.As an example,the dependence of c2onλfor L t=3is shown infig.2.To determine the critical value ofλi.e.the largest value,where c2=0,we have performedfits linear inλto the nonnegative c2 values.Figure1.Dependence of c2onλfor L t=3. Having determined the endpointλcrit.(L t)for each L t we calculate the T=0quantities (R HW,g2R)on V=(32L t)·(8L t)·(6L t)3lattices, where32L t belongs to the temporal extension, and extrapolate to the continuum limit.Having established the correspondence betweenλcrit.(L t) and R HW,the L t dependence of the critical R HW is easily obtained.Fig.3shows the dependence of the endpoint R HW values on1/L2t.A linear extrapolation in1/L2t yields the continuum limit value of the endpoint R HW.We obtain66.5±1.4 GeV,which is ourfinal result.Comparing our result to those of the3d anal-yses[9]one observes complete agreement.Since the error bars on the endpoint determinations are on the few percent level,the uncertainty of the dimensional reduction procedure is also in this range.This indicates that the analogous per-turbative inclusion of the fermionic sector results also in few percent error on M H.Based on our published data[4,11]and the present results we are able to draw the phase dia-gram of the SU(2)-Higgs model in the(T c/m H−R HW)plane.This is shown infig. 4.The con-tinuous line–representing the phase-boundary–is a quadraticfit to the data points.Finally,we determine what is the endpoint value in the full SM.Our nonperturbative anal-3Figure 2.Dependence of R HW,cr ,i.e.R HW cor-responding to the endpoint of first order phase transitions on 1/L 2t and extrapolation to the in-finite volumelimit.Figure 3.Phase diagram of the SU(2)-Higgs model in the (T c /m H −R HW )plane.ysis shows that the perturbative integration of the heavy modes is correct within our error bars.Therefore we use perturbation theory [13]to transform the SU(2)-Higgs model endpoint value to the full SM.We obtain 72.4±1.7GeV,where the error includes the measured error ofR HW,cont.,g 2R and the estimated uncertainty [14]due to the different definitions of the gauge cou-plings between this paper and [13].The dominant error comes from the uncertainty on the position of the endpoint.The present experimental lower limit of the SM Higgs-boson mass is 89.8GeV [15].Taking into account all errors (in particular those coming from integrating out the heavy fermionic modes),our endpoint value excludes the possibility of any EWPT in the SM.This also means that the SM baryogenesis in the early Universe is ruled out.For details of this analysis see [16].Simulations have been carried out on the Cray-T90at HLRZ-J¨u lich,on the APE-Quadrics at DESY-Zeuthen and on the PMS-8G PC-farm in Budapest.This work was supported by OTKA-T016240/T022929and FKP-0128/1997.REFERENCES1.V.A.Kuzmin,V.A.Rubakov and M.E.Sha-poshnikov,Phys.Lett.B155(1985)36.2.W.Buchm¨u ller at al.,Ann.Phys.(NY)234(1994)260;Z.Fodor, A.Hebecker,Nucl.Phys.B432(1994)127.3. B.Bunk,E.M.Ilgenfritz,J.Kripfganz,A.Schiller,Nucl.Phys.B403(1993)453.4. F.Csikor et al.Nucl.Phys.B474(1996)421and references therein.5.K.Kajantie,K.Rummukainen,M.E.Sha-poshnikov,Nucl.Phys.B407(1993)356.6.K.Kajantie at al.,Nucl.Phys.B493(1997)413and references therein.7. F.Csikor,Z.Fodor and J.Heitger,hep-lat/9807021.8.K.Kajantie at al.,Phys.Rev.Lett.77(1996)2887;K.Rummukainen et al.,hep-lat/9805013.9. F.Karsch et al.Nucl.Phys.Proc.Suppl.53(1997)623;M.G¨u rtler,E.M.Ilgenfritz,A.Schiller,Phys.Rev.D56(1997)3888;for a recent review with references see:ine,in Proc.SEWM’97,Eger,Hungary,May 1997,World Sci,1998,p.160.10.F.Csikor and Z.Fodor,Phys.Lett.B380(1996)113.11.F.Csikor,Z.Fodor and J.Heitger,hep-lat/9804026.12.C.N.Yang and T. D.Lee,Phys.Rev.87(1952)404.13.K.Kajantie at al.,Nucl.Phys.B466(1996)189.ine,Phys.Lett.B385(1996)249.15.P.McNamara,talk given at the ICHEP’98.16.F.Csikor,Z.Fodor and J.Heitger,hep-ph/9809291.。

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