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is not true regardless of convention for the standard form of those metrics. Please state your sources.Tanujhm said:Summary: FLRW
despite Minkowskis, Schwarzschilds and Kerrs
Right, my fault.Orodruin said:Ah no wait:
This
is not true regardless of convention for the standard form of those metrics. Please state your sources.
... and the metric signature is not the only sign convention so beware of the others too!Ibix said:if they use different conventions you can find inconsistent signs
I don't understand what you are trying to say here. Using an exact FLRW metric as an approximation for our actual universe on large scales is not the same as claiming that the exact FLRW metric you are using is an exact solution for more than one set of initial conditions. It's just an approximation.Dragrath said:There is an alarming fallacious tendency in cosmology to assume that you can approximate a universe under the FLRW metric if you have sufficiently small deviations from perfect isotropy such that you can treat the universe as uniform ans isotropic at large scales but this would require a violation of the conservation of information which must hold mathematically for any system of partial differential equations since by definition there must be a unique solution for all possible valid initial conditions.
I have no idea where you are getting this from. There are many other exact solutions known:Dragrath said:the FLRW metric remains the only known exact solution to the general Einstein field equations
Do you mean this paper?Dragrath said:Matthew Kleban and Leonardo Senatore JCAP10(2016)022
This claim is much too strong; see my comments above. I don't think the paper you reference supports it either, particularly since the only scenario that paper claims to rule out, the "Big Crunch", is not part of our best current model of our universe anyway.Dragrath said:The point of the above is that we have already mathematically falsified the validity of FLRW based cosmology by showing it requires the violation of information conservation making any such solutions mathematically invalid.
Do you mean this paper?Dragrath said:Nathan J. Secrest et al 2021 ApJL 908 L51
This claim is much too strong as well. See my remarks above about approximation.Dragrath said:Nowadays we have amassed more than enough observational proof to falsify the cosmological principal (Nathan J. Secrest et al 2021 ApJL 908 L51) as well as theoretical reasons for why the cosmological principal must always be violated yet in cosmology FLRW is still taken as gospel in the form of Lambda CDM cosmology.
The Robertson-Walker metric is a mathematical framework used to describe the geometry of the universe in the context of general relativity. It is a solution to Einstein's field equations and is used to model the expansion of the universe.
The Robertson-Walker metric is derived from the Friedmann-Lemaitre-Robertson-Walker (FLRW) metric, which is a generalization of the Friedmann equations. It takes into account the curvature of space and the expansion of the universe.
The Robertson-Walker metric assumes that the universe is homogeneous and isotropic, meaning that it is the same in all directions and at all points in space. It also assumes that the universe is expanding, but not accelerating.
The Robertson-Walker metric is used to describe the large-scale structure of the universe and to make predictions about its evolution. It is also used to calculate important quantities such as the Hubble parameter and the scale factor, which are used in cosmological models.
While the Robertson-Walker metric is a useful tool in cosmology, it has some limitations. It does not take into account the effects of dark energy, dark matter, or gravitational waves, which are important factors in the evolution of the universe. It also assumes a flat universe, which may not be accurate for our actual universe.