B Types of Metrics: Background & Reference Explained

  • B
  • Thread starter Thread starter windy miller
  • Start date Start date
windy miller
Messages
306
Reaction score
28
As I understand it relativity is built using a mathematical framework called a metric. ButI have heard some scientists refer to things like a background metric and a reference meteoric. Can anyone explain what these are?
 
Physics news on Phys.org
Background metric is used to consider the motion of a body considered to be 'small'. In the simplest case, the small body is treated as a 'test particle' moving as a geodesic in the background metric. On the other hand, to consider backreaction from gravitational wave emission without the full machinery of numerical relativity, the small body is considered to provide a metric perturbation on top of the background metric. These are just approximation techniques. They do not suggest there are really different types of metrics in the theory of General Relativity.

I have not heard of the term 'reference metric', so I can't answer that question.
 
  • Like
Likes vanhees71
PAllen said:
Background metric is used to consider the motion of a body considered to be 'small'. In the simplest case, the small body is treated as a 'test particle' moving as a geodesic in the background metric. On the other hand, to consider backreaction from gravitational wave emission without the full machinery of numerical relativity, the small body is considered to provide a metric perturbation on top of the background metric. These are just approximation techniques. They do not suggest there are really different types of metrics in the theory of General Relativity.

I have not heard of the term 'reference metric', so I can't answer that question.
thanks
 
In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
Thread 'Dirac's integral for the energy-momentum of the gravitational field'
See Dirac's brief treatment of the energy-momentum pseudo-tensor in the attached picture. Dirac is presumably integrating eq. (31.2) over the 4D "hypercylinder" defined by ##T_1 \le x^0 \le T_2## and ##\mathbf{|x|} \le R##, where ##R## is sufficiently large to include all the matter-energy fields in the system. Then \begin{align} 0 &= \int_V \left[ ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g}\, \right]_{,\nu} d^4 x = \int_{\partial V} ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g} \, dS_\nu \nonumber\\ &= \left(...
Abstract The gravitational-wave signal GW250114 was observed by the two LIGO detectors with a network matched-filter signal-to-noise ratio of 80. The signal was emitted by the coalescence of two black holes with near-equal masses ## m_1=33.6_{-0.8}^{+1.2} M_{⊙} ## and ## m_2=32.2_{-1. 3}^{+0.8} M_{⊙}##, and small spins ##\chi_{1,2}\leq 0.26 ## (90% credibility) and negligible eccentricity ##e⁢\leq 0.03.## Postmerger data excluding the peak region are consistent with the dominant quadrupolar...
Back
Top