In General
* History: 1934, Born-Infeld
theory can be considered as a form of bimetric theory (according to Moffat);
1973–1974, New version proposed by N Rosen;
1979–1995,
J Moffat's non-symmetric gravitation theory; 1992, J Bekenstein's
treatment
of gravitational lensing and MOND; 1998–2003, Clayton-Moffat scalar-vector-tensor
theory.
* Setup: If we call gab the gravitational metric, which
controls the speed of gravity, a second metric is given by
g'ab = gab +
(B/c2)
a
b
,
where B is a positive number (which will probably be renormalized
by quantum effects), and
a
scalar field coupled to gravity (gab);
All other fields couple to the "matter metric" g'ab,
whose light
cones therefore control their propagation.
* Properties: One of
the main differences with general relativity is that it does not produce
black holes.
Phenomenology > s.a. anomalous
acceleration; variation
of constants; [cosmological models].
* Variation of c: The different metrics that apply to gravitation
and other fields give rise to an effectively changing speed of light; Depending
on
whether
one uses electromagnetic or other (say, gravitational) waves to study
the
early universe, one gets that the other speed changes in time (the ratio cgrav/cgamma
is dimensionless and meaningful).
* Cosmology: If we set
the gravitational cgrav to
be constant, the electromagnetic cgamma will
vary and increase close to the
big bang;
This
solves the horizon problem without using inflation (although the Friedmann
equation
changes too).
@ References: Moffat ap/00,
IJMPD(03)gq/02 [variable c and
supernovas]; Moffat qp/02 [entanglement];
Kopeikin & Ni gq/06-in
[laser ranging delay]; Kopeikin gq/05 [speed
of light and gravity]; Petit & D'Agostini a0712 [and
cosmological acceleration]; Bañados et al PRD(09)-a0811
[and dark matter].
References
@ General: Rosen AP(63), AP(66)
[with flat metric], GRG(73),
AP(74), & Rotbart GRG(79);
Drummond PRD(01)ap/00 [dark
matter
alternative]; Leiter & Robertson gq/01/GRG
[?]; Pitts & Schieve
GRG(01)gq ["slightly
bimetric"], gq/01-in
[consistency]; Blas et al PRD(07);
Afshar a0910 [3-dimensional].
@ Related topics:
Damour & Kogan PRD(02)
[non-linear, Leff]; Blas
et al CQG(06)
[solutions, causal structure]; Hohmann & Wohlfarth a0908 [positive and negative
mass].
@ Multigravity: Kogan ap/01-in
[overview].
@ Other variants: Pitts & Schieve FP(04)
[in Minkowski, same light cones]; Hossenfelder PRD(08)-a0807 [with
exchange symmetry].
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send feedback and suggestions to bombelli at olemiss.edu – modified 22
oct 2009