In General > s.a. scalar-tensor
theories.
* Idea: A scalar-tensor
theory of gravity containing an arbitrary "Dicke coupling constant"
.
* In the Jordan frame:
The action, if K (K0) is the
trace of the extrinsic curvature induced by g (
)
on
M
and including
a cosmological constant, is
SJ[g,
,
...] = (1/16
)
M
dv [
(R – 2
) –
gab
–1
a
b
]
+ 2
bdry(M)
(
K–
0K0)
ds + Smatter ;
The field equations, in units in which G = 1, are
![]()
=
{8
/3 + 2
) T , Gab
= (8![]()
–1)Tab
+ (![]()
–2)
(
,a
,b
–
gab
,m
,m)
+
–1
(
;ab – gab ![]()
)
.
* In the Einstein frame: The action is
SE[g,
,
...] = (1/16
)
M dv [R – (
+
3/2)
,a
,a]
+
M dv exp{–2
}
m ;
The field equations are
Gab =
8
(
,a
,b
–
gab gmn
,m
,n)
.
* History: Perfectly viable in 1971, was neglected for some years, then revived since the 1980s because it (with other matter fields) arises in Kaluza-Klein theories, and as an effective theory in the low-energy limit of string theory.
Phenomenology > s.a.
cosmic acceleration; early-universe
cosmology; gravitomagnetism; monopoles; wormhole
solutions.
* Properties: The massless
is
to be thought of as corresponding to
a "varying gravitational constant G
–1";
It incorporates the weak form of the equivalence principle, not the strong
one; The local special relativistic
laws are valid as usual; The field
interacts
with matter only indirectly, through
the metric.
* Bounds: 1973, needed
> 5
for reasonable agreement with experiment; 1987, There are much stronger lower
bounds, and it does not seem very
natural (the
→
limit
of the theory is general relativity, if Taa
0).
* And PPN parameters:
Cosmological models predict a departure from the general relativity value of
|1–
|
between 10–5 and
10–7.
@ Tests, effects: Dereli & Tucker MPLA(02)gq/01 [precession
and torsion]; Barros & Romero MPLA(03)
[time delay & Lense-Thirring
effect]; Psaltis ap/05/ApJ
[msec pulsars]; Carneiro & Montenegro BJP(05)gq-in
[and cosmic coincidence].
@ Gravitational waves: Scharre & Will PRD(02)gq/01 [waveforms];
Sahoo & Singh
MPLA(04)gq;
Will & Yunes CQG(04)gq [and
LISA]; Faraoni PRD(04)gq [negative
energy,
stability of Minkowski]; > s.a. gravitational-wave
background; scalar-tensor
theories.
@ Topological defects: Barros & Romero PRD(97)
[monopoles], MPLA(01)
[gravitational forces]; Dahia & Romero PRD(99)gq/98 [lines];
Delice PRD(06)gq,
PRD(06)
[cosmic
strings, with cosmological constant].
@ Black holes: Campanelli & Loustó IJMPD(93)gq;
Beesham MPLA(98)
[parameter interpretation]; Tamaki et al PRD(98)gq/97 [non-abelian],
PRD(99)gq [monopole];
Kim PRD(99)
[Kerr-Newman type]; Agnese & La Camera NCB(01)gq/00 [black
hole
metric
fluctuations]; Sakai & Barrow CQG(01)gq [evolution];
Kozyrev gq/02 [static,
spherical]; Sheykhi & Alavirad IJMPD-a0809 [Brans-Dicke-Maxwell];
Avelino et al PRD(09)-a0904 [mass
inflation].
@ Bianchi models: Guzman
PLB(97)
[cosmic no-hair theorem]; Cervantes-Cota & Nahmad GRG(01)gq/00 [I-V-IX,
solutions and isotropization]; Núñez-Yépez GRG(01)
[VII]; > s.a. bianchi
models; chaos in bianchi models; inflationary
models.
@ Inflation:
Gong
PRD(99)gq/98; del
Campo et al JCAP(07)
[emergence from past-eternal
static spacetime]; Berman & Trevisan IJTP(09)gq/01.
@ Other FRW cosmology: Wetterich NPB(88)
[varying G]; Gong gq/98;
Quirós et al PRD(00)
[singularity]; Arik & Çalik MPLA(06)gq/05 [dark
energy
and dark matter]; Arik et al IJMPD(08)gq/06 [Friedmann
equation]; Berman gq/06/ASS;
Montenegro & Carneiro CQG(07)gq/06 [decaying
vacuum density].
@ Other cosmology: Krori et al PLA(81)
[stationary axisymmetric Brans-Dicke-Maxwell];
Pimentel
PRD(96),
MPLA(97);
Park & Sin
JKPS(99)gq;
Chen et al IJTP(05)gq/03 [and
Higgs mechanism]; Acquaviva & Verde JCAP(07)-a0709 [and
cosmological parameters]; Smolyakov a0711 [and
small cosmological constant]; del Campo et al JCAP(09)
[static universe,
stability]; > s.a. NUT Space; singularities.
References > s.a. 3D gravity; gravitational
constant;
quantum cosmology;
quintessence.
@ General: Brans & Dicke PR(61);
Dicke PR(62);
in Dicke 64; Jackiw NC(68).
@ Summaries: in Misner et al 73, 1070ff; Will in(79).
@
→
limit:
Banerjee & Sen PRD(97); Faraoni PLA(98)gq,
PRD(99)gq;
Quirós gq/99/PLA;
Bhadra & Nandi PRD(01)gq/04 [scalar field]; Chauvineau CQG(03).
@
→ 0 limit:
Punzi et al PLB(08)-a0804 [geometrical
structure].
@ Quantum theory: Cho CQG(97)
[and equivalence principle]; Zhu et al MPLA(98)
[quantum cosmology and cosmological constant]; Pimentel & Mora PLA(01)gq/00 [3rd
quantization]; Ohkuwa NCB(03)
[WKB time]; > s.a. renormalization of quantum
gravity.
@ Generalizations, extensions: Chakraborty & Ghosh PS(03);
Catena PRD(07)ht/06 [minimal
supersymmetric extension]; Amendola et al PRD(08)-a0801 [with
Gauss-Bonnet term, and Solar System tests]; Smolyakov a0907 [non-linear,
Born-Infeld-like]; Qiang et al PLB(09) [5D, and cosmology].
@ Related topics: Arazi & Simeone MPLA(00)gq [linearized,
strings]; Miyazaki gq/00/PRD
[and general relativity]; Bhadra et al MPLA(07)
[Jordan vs Einstein frame]; Rador PLB(07)
[Brans-Dicke type higher-order gravity]; Chernodub & Niemi PRD(08)-a0709 [and
electroweak
theory]; Faraoni CQG(09)-a0906 [mass
and range of scalar field]; > s.a. spherical
general relativity.
main page – abbreviations – journals – comments – other
sites – acknowledgements
send feedback and suggestions to bombelli at olemiss.edu – modified 24
oct 2009