2017
DOI: 10.1088/1361-6382/aa83d4
|View full text |Cite
|
Sign up to set email alerts
|

Torsional Newton–Cartan gravity from the large c expansion of general relativity

Abstract: We revisit the manifestly covariant large c expansion of General Relativity, c being the speed of light. Assuming the relativistic connection has no pole in c −2 , this expansion is known to reproduce Newton-Cartan gravity and a covariant version of Post-Newtonian corrections to it. We show that relaxing this assumption leads to the inclusion of twistless torsion in the effective non-relativistic theory. We argue that the resulting TTNC theory is an effective description of a non-relativistic regime of General… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

7
221
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
8
1

Relationship

0
9

Authors

Journals

citations
Cited by 103 publications
(228 citation statements)
references
References 19 publications
(69 reference statements)
7
221
0
Order By: Relevance
“…This has severe implications: the result of gauging the Bargmann algebra will in general not coincide with the 1/c 2 expansion of general relativity [2]! To see how strong field effects are encoded into the non-relativistic limit of general relativity, we define the following covariant 1/c 2 expansion (where c is the slope of the light cone in tangent space) of the Lorentzian metric 1 g µν [3,12]:…”
mentioning
confidence: 99%
“…This has severe implications: the result of gauging the Bargmann algebra will in general not coincide with the 1/c 2 expansion of general relativity [2]! To see how strong field effects are encoded into the non-relativistic limit of general relativity, we define the following covariant 1/c 2 expansion (where c is the slope of the light cone in tangent space) of the Lorentzian metric 1 g µν [3,12]:…”
mentioning
confidence: 99%
“…Above we used the boost invariant covariant derivatives (3.13). We may fix arbitrary coefficients in equations (5.4) by comparing it with a similar result in [33]. In four dimensions (d = 3) the similar equation of [33] is;…”
Section: Ehlers Conditionsmentioning
confidence: 97%
“…In the presence of twistless torsion i.e. b a = 0 the equations of motion are given in [1,33,34]. In [1] these equations were obtained by exploiting the non-relativistic conformal method starting from a Schrödinger field theory in flat spacetime.…”
Section: Poisson's Equationmentioning
confidence: 99%
“…These conditions do not depend on the choice of longitudinal frame and, thus, they refer to the structure of the metrics τ and h. In fact, when studying pNC geometries as the leading terms of a covariant expansion of General Relativity [26][27][28], it is useful to rewrite the results in Proposition 3.2 in terms of such metrics and in a general coordinate chart as follows…”
Section: The Equivalence Problem In Non-relativistic Structuresmentioning
confidence: 99%