An introduction to the physics of Cartan gravity

被引:20
作者
Westman, Hans F. [1 ]
Zlosnik, Tom G. [2 ]
机构
[1] CSIC, Inst Fis Fundamental, Madrid 28006, Spain
[2] Imperial Coll Theoret Phys, London SW7 2AZ, England
关键词
Modified gravity; Cosmology; GAUGE-THEORY; SIGNATURE; BREAKING; FIELDS;
D O I
10.1016/j.aop.2015.06.013
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
A distance can be measured by monitoring how much a wheel has rotated when rolled without slipping. This simple idea underlies the mathematics of Cartan geometry. The Cartan-geometric description of gravity consists of a SO(1, 4) gauge connection A(AB) (x) and a gravitational Higgs field V-A (x) which breaks the gauge symmetry. The clear similarity with symmetry-broken Yang-Mills theory suggests strongly the existence of a new field VA in nature: the gravitational Higgs field. By treating V-A as a genuine dynamical field we arrive at a natural generalization of General Relativity with a wealth of new phenomenology. Importantly, General Relativity is reproduced exactly in the limit that the SO(1, 4) norm V-2 (x) tends to a positive constant. We show that in regions wherein V-2 varies - but has a definite sign - the Cartan-geometric formulation is a particular version of a scalar-tensor theory (in the sense of gravity being described by a scalar field phi, metric tensor g(mu nu), and possibly a torsion tensor T-mu nu(rho)). A specific choice of action yields the Peebles-Ratra quintessence model whilst more general actions are shown to exhibit propagation of torsion. Regions where the sign of V-2 changes correspond to a change in signature of the geometry. Specifically, a simple choice of action with FRW symmetry imposed yields, without any additional ad hoc assumptions, a classical analogue of the Hartle-Hawking no-boundary proposal with the big bang singularity replaced by signature change. Cosmological solutions from more general actions are described, none of which have a big bang singularity, with most solutions reproducing General Relativity, or its Euclidean version, for late cosmological times. Requiring that gravity couples to matter fields through the gauge prescription forces a fundamental change in the description of bosonic matter fields: the equations of motion of all matter fields become first-order partial differential equations with the scalar and Dirac actions taking on structurally similar first-order forms. All matter actions reduce to the standard ones in the limit V-2 -> const. We argue that Cartan geometry may function as a novel platform for inspiring and exploring modified theories of gravity with applications to dark energy, black holes, and early-universe cosmology. We end by listing a set of open problems. (C) 2015 Elsevier Inc. All rights reserved.
引用
收藏
页码:330 / 376
页数:47
相关论文
共 58 条
[1]   Chern-Simons modified general relativity [J].
Alexander, Stephon ;
Yunes, Nicolas .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2009, 480 (1-2) :1-55
[2]   Chern-Simons modified gravity as a torsion theory and its interaction with fermions [J].
Alexander, Stephon ;
Yunes, Nicolas .
PHYSICAL REVIEW D, 2008, 77 (12)
[3]  
Anderson J.L., 1967, Principles of relativity physics
[4]  
[Anonymous], GRQC0606062
[5]   Relativistic gravitation theory for the modified Newtonian dynamics paradigm [J].
Bekenstein, JD .
PHYSICAL REVIEW D, 2004, 70 (08)
[6]  
Blagojevic M., 2002, STUD HI ENER PHY COS
[7]   Barbero-Immirzi field in canonical formalism of pure gravity [J].
Calcagni, Gianluca ;
Mercuri, Simone .
PHYSICAL REVIEW D, 2009, 79 (08)
[8]   MASSIVE SUPERGRAVITY FROM SPONTANEOUSLY BREAKING ORTHOSYMPLECTIC GAUGE SYMMETRY [J].
CHAMSEDDINE, AH .
ANNALS OF PHYSICS, 1978, 113 (01) :219-234
[9]   Who ordered the anti-de Sitter tangent group? [J].
Chamseddine, Ali H. ;
Mukhanov, Viatcheslav .
JOURNAL OF HIGH ENERGY PHYSICS, 2013, (11)
[10]   Cosmological dynamics with propagating Lorentz connection modes of spin zero [J].
Chen, Hsin ;
Ho, Fei-Hung ;
Nester, James M. ;
Wang, Chih-Hung ;
Yo, Hwei-Jang .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2009, (10)