Topological Gravity, Kaluza-Klein Reduction, and the Kink

Topological Gravity, Kaluza-Klein Reduction, and the Kink
Topological Gravity, Kaluza-Klein Reduction, and the Kink

a r X i v :h e p -t h /0401124v 2 2 M a r 2004

MIT-CTP-3467hep-th/0401124

Topological Gravity,Kaluza-Klein Reduction,and the Kink 1

Alfredo Iorio

Center for Theoretical Physics,Massachusetts Institute of Technology

77,Massachusetts Avenue -Cambridge MA 02139USA

Abstract

Kaluza-Klein reduction of the 3d gravitational Chern-Simons term leads to a 2d theory that supports a symmetry breaking solution and an associated kink interpolating between AdS and dS geometries.

1Chern-Simons Gravity

Chern-Simons (CS)gauge theories,either pure or as modi?cations of Yang-Mills theories,have been studied from a variety of perspectives,gravity included.Nonetheless,some aspects of the impact on gravity deserve further investigation.

The probably best known arena for CS gravity is in 3dimensions[2]

GR(G μν)=

d 3x

√4π2

d 3x?

μνλ

1

3

ΓρμσΓσντΓτ

λρ

.(2)

This leads to a topologically massive scalar graviton theory,descending from the theory GR(G μν)+

1/μCS(Γ).

In the ?rst order formulation of Vielbein (E A μ)and spin connections (?AB μ

)the gauge theoretical nature of 3d gravity becomes more transparent.Treating E and ?as independent variables,it was proved the equivalence[4]GR(E,?)?CS(E,?).This only happens in 3dimensions,where a non-degenerate,ISO(2,1)-invariant,bilinear form can be de?ned in terms of P A and J A ,generators of translations and rotations,respectively.The Dreibein is the gauge ?eld associated

to P A,while the spin connection is the gauge?eld associated to J A.A di?erent perspective takes?(E),obtained imposing torsionlessness rather than having it has an Euler-Lagrange(EL) equation.On this see,for instance,[5].

2Kaluza-Klein Reduction

We shall concentrate on CS(Γ)alone and dimensionally reduce it in a Kaluza-Klein(KK)

setting[1].We have

δCS(Γ)=?1

GCμνδGμν,(3)

where the Cotton tensor Cμν,de?ned by

Cμν=?1

??xμ U?1Aσ(x)U+U?1?

4π2 d3x?μνλ

tr 13?μ?ν?λ ?1

term,while this is not the case for the gravity term[7].We shall not consider W(E)any further. In3d?μ,AB=?ABC?Cμ,thus

CS(?)=?1

2π2 d3x det?Aμ.(8)

With the KK Ansatz the3d metric tensor reads(see for instance[8])

Gμν=φ gαβ?aαaβ?aα

?aβ?1

,(9)

where all quantities are independent of y,and,transforming Gμνunderδxμ=?ξμ(t,x),it is seen that gαβis the2d metric tensor,aαis a2d gauge vector,(α,β=0,1),andφis a scalar. As the CS term is conformally invariant we setφ=1.

The reduced Dreibein E Aμand spin connection?Aμread

E aα=e aα,E2α=aα,E a2=0,E22=1,(10)

?aα=1

2

faα,?a2=0,?22=?

1

?g?αβf,where fαβ=?[αaβ].

With these,the dimensionally reduced gravitational CS term is eventually obtained

CS=?1

?g(fr+f3),(12)

where g=det gαβ,and r is the2d scalar curvature.

The3d scalar curvature R with the KK Ansatz(andφ=1)reduces to

R=r+

1

4π2 d2x√2Tαβδgαβ),(14) where jα=?(1/2√2rf)?DαDβf.As a consequence of gauge and2d di?eo invariance Dαjα=0,and DβTαβ=0,respectively.The components of the dimensionally reduced Cotton tensor are Cαβ=Tαβ,Cα2=?jα?Tαβaβ, and C22=gαβTαβ+aαTαβaβ+2jαaα.Thus the EL equations are

?αβ?β(r+3f2)=0,gαβ(D2f?f3?1

The?rst is solved by r+3f2=constant=c.Eliminating r in the second equation,and decomposing into the trace and trace-free parts lead to

0=D2f?cf+f3,(16)

0=DαDβf?

1

c,r=?2c, (c>0),with R=?(3/2)c.The latter is maximally symmetric,the former is not.

When the symmetry breaking solution is present,there also is a kink solution

f=

√c

c,and giving rise to r=?2c+3c/(cosh2√

2

x),with3d scalar

curvature R=?3c/2+5c/(2cosh2√

2 x).

The global properties of the reduced theory above described have been now extensively studied[9]. 4Overview

There are various dimensional reductions/enhancements one can perform on the CS gravity term:3d→2d[this work,[1]];4d←3d[10];(2N+1)d→2Nd in particular5d→4d[11]. References

[1]G.Guralnik,A.Iorio,R.Jackiw,S.-Y.Pi,Ann.Phys.308(2003)222.

[2]S.Carlip,Quantum gravity in2+1dimensions,Cambridge University Press(1998).

[3]S.Deser,R.Jackiw,S.Templeton,Ann.Phys.(NY)140(1982)372.

[4]E.Witten,Nucl.Phys.B311(1988/89)46.

[5]J.H.Horne,E.Witten,Phys.Rev.Lett.62(1989)501.

[6]A.Garcia,F.W.Hehl,C.Heinicke,A.Macias,The Cotton tensor in Riemannian spacetimes,

gr-qc/0309008.

[7]R.Percacci,Ann.Phys.177(1987)27.

[8]L.O’Raifeartaigh,N.Straumann,Rev.Mod.Phys.72N.1(2000).

[9]D.Grumiller,W.Kummer,Ann.Phys.308(2003)211.

[10]R.Jackiw,S.-Y.Pi,Phys.Rev.D68(2003)10412.

[11]D.Grumiller,A.Iorio,in preparation.

4

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而且这些属性是可以多选的,用“|”分开。 默认这个的值是:Gravity.LEFT 对这些属性的描述: 出自: https://www.360docs.net/doc/5610885282.html,/guide/topics/resources/drawable-res ource.html https://www.360docs.net/doc/5610885282.html,/reference/android/graphics/drawable /ClipDrawable.html Value Description top Put the object at the top of its container, not changing its size. 将对象放在其容器的顶部,不改变其大小. bottom Put the object at the bottom of its container, not changing its size. 将对象放在其容器的底部,不改变其大小.

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东亚贸易gravity model应用-国际经济学

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I.Introduction E CONOMISTS have long been aware that Jensen’s in- equality implies that E(ln y) ln E(y),that is,the expected value of the logarithm of a random variable is different from the logarithm of its expected value.This basic fact,however,has been neglected in many economet-ric applications.Indeed,one important implication of Jen-sen’s inequality is that the standard practice of interpreting the parameters of log-linearized models estimated by ordi-nary least squares(OLS)as elasticities can be highly mis-leading in the presence of heteroskedasticity. Although many authors have addressed the problem of obtaining consistent estimates of the conditional mean of the dependent variable when the model is estimated in the log linear form(see,for example,Goldberger,1968;Man-ning&Mullahy,2001),we were unable to?nd any refer-ence in the literature to the potential bias of the elasticities estimated using the log linear model. In this paper we use the gravity equation for trade as a particular illustration of how the bias arises and propose an appropriate estimator.We argue that the gravity equation, and,more generally,constant-elasticity models,should be estimated in their multiplicative form and propose a simple pseudo-maximum-likelihood(PML)estimation technique. Besides being consistent in the presence of heteroskedas-ticity,this method also provides a natural way to deal with zero values of the dependent variable. Using Monte Carlo simulations,we compare the perfor-mance of our estimator with that of OLS(in the log linear speci?cation).The results are striking.In the presence of heteroskedasticity,estimates obtained using log-linearized models are severely biased,distorting the interpretation of the model.These biases might be critical for the compara-tive assessment of competing economic theories,as well as for the evaluation of the effects of different policies.In contrast,our method is robust to the different patterns of heteroskedasticity considered in the simulations. We next use the proposed method to provide new esti-mates of the gravity equation in cross-sectional https://www.360docs.net/doc/5610885282.html,ing standard tests,we show that heteroskedasticity is indeed a severe problem,both in the traditional gravity equation introduced by Tinbergen(1962),and in a gravity equation that takes into account multilateral resistance terms or?xed effects,as suggested by Anderson and van Wincoop(2003). We then compare the estimates obtained with the proposed PML estimator with those generated by OLS in the log linear speci?cation,using both the traditional and the?xed-effects gravity equations. Our estimation method paints a very different picture of the determinants of international trade.In the traditional gravity equation,the coef?cients on GDP are not,as gen-erally estimated,close to1.Instead,they are signi?cantly smaller,which might help reconcile the gravity equation with the observation that the trade-to-GDP ratio decreases with increasing total GDP(or,in other words,that smaller countries tend to be more open to international trade).In addition,OLS greatly exaggerates the roles of colonial ties and geographical proximity. 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Despite the focus on the gravity equation,our criticism of the conventional practice and the solution we propose ex-tend to a broad range of economic applications where the equations under study are log-linearized,or,more generally, transformed by a nonlinear function.A short list of exam-ples includes the estimation of Mincerian equations for wages,production functions,and Euler equations,which are typically estimated in logarithms. Received for publication March29,2004.Revision accepted for publi- cation September13,2005. *ISEG/Universidade Te′cnica de Lisboa and CEMAPRE;and London School of Economics,CEP,and CEPR,respectively. We are grateful to two anonymous referees for their constructive comments and suggestions.We also thank Francesco Caselli,Kevin Denny,Juan Carlos Hallak,Daniel Mota,John Mullahy,Paulo Parente, Manuela Simarro,and Kim Underhill for helpful advice on previous versions of this paper.The usual disclaimer applies.Jiaying Huang provided excellent research assistance.Santos Silva gratefully acknowl- edges the partial?nancial support from Fundac?a?o para a Cie?ncia e Tecnologia,program POCTI,partially funded by FEDER.A previous version of this paper circulated as“Gravity-Defying Trade.” The Review of Economics and Statistics,November2006,88(4):641–658 ?2006by the President and Fellows of Harvard College and the Massachusetts Institute of Technology

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document公文,文件midnight午夜,半夜bored厌烦的,不感兴趣的 ----------------------- Lesson2 stress压力studio工作室,演播室expert专家suffer感到疼痛,遭受(痛苦) suffer from忍受,遭受social爱交际的;社交的organize组织 stand忍耐,忍受 volunteer志愿者minus负,零下challenge挑战 dial拨(电话号码) advertisement广告solve解答,解决 accountant会计,会计师crowded拥挤的otherwise否则,另外crowd人群,一伙人distance距离sickness疾病 pressure压力 reduce减少降低 diet饮食,节食 prefer更喜欢,宁愿 ----------------------- Lesson3 graduate毕业 basin水盆,脸盆 support&支持;支撑 design&设计 presentation表演,展示 ----------------------- Lesson4 tube(英)地铁 nearby附近的;在附近 forecast预测,预报 lung肺 distance learning远程学习 cigar雪茄烟

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