PAllen said:
This is all mixed up. Lambd-CDM is a full GR cosmology model. There is no approximation whatsoever in all its defining equations; it is fully non-linear. To perform some types of calculations more easily, one sometimes approximates the full model in various ways.
In practice, at the scale of galaxies and galaxy clusters, Lambda-CDM is approximated with Newtonian gravity.
PAllen said:
MOND has no relation to GR, it is (in its original form) a modifications to Newtonian mechanics that happens to explain a bunch of esp. galactic observations. It is generally treated as suggestive of the idea that more plausible modified gravity theories are worth pursuing (in itself, in the original form, it is worthless because it fails to match any of the dozens of verified GR predictions that differ from Newtonian.
MOND proponents are not GR deniers in strong gravitational fields. These are PhD astronomers who fully endorse and accept the experimental validations of GR to date as true and correct.
MOND proponents are merely advocates for a second order gravitational effect (whose deeper mechanism and exactly functional form are unknown) in addition to GR as conventionally applied in very weak gravitational fields in circumstances where no significant external fields are present encompassing the whole system.
MOND proponents do assert that external field effect in MOND (in which two bodies that would have an enhanced MOND gravitational attraction since the Newtonian acceleration between them would be very weak do not do so when a gravitational field external to the two free falling bodies from something like a nearby galaxy is present at a strength greater than the MOND acceleration constant) contradicts the strong equivalence principle of GR, as supported by statistical evidence from many galaxy observations. See
arXiv:2009.11525 (published in ApL in 2020). This is
not contrary to any precision tests of GR.
People who are using MOND are implicitly only using it in a domain of applicability where a Newtonian approximation of GR would be used instead. They readily assume that significantly above the a
0 threshold that GR is actually what applies.
Likewise, other assumptions of GR (e.g. that light is bent by gravitational fields in proportion to the strength of the gravitational field in both the MOND and non-MOND regimes to the same extent as it would be in GR) are also assumed.
MOND is agnostic on the existence of the cosmological constant or dark energy whose existence depends upon observations outside of its domain of applicability. Nothing about MOND is inherently inconsistent with the cosmological constant of GR, but MOND, since it is agnostic about the mechanism by which this effect arises, also does not require a cosmological constant or dark energy to explain the predictions it makes in its domain of applicability.
Criticizing MOND for failure to match GR predictions is a straw man fallacy that misunderstands what the theory really is. There are several relativistic generalizations of MOND that explicitly incorporate GR effects in the appropriate domains of applicability.
There are legitimate grounds to criticize simple toy-model MOND and its relativistic generalizations. The most widely known and acknowledged flaw of MOND is that it underestimates the magnitude of dark matter phenomena in galaxy clusters and doesn't scale the magnitude of dark matter phenomena in galaxy clusters with the right exponent, even though it partially captures these effects. But these flaws don't cure the many known flaws of other theories that also get lots of things wrong like LambdaCDM.
From a phenomenology perspective, Deur brings three main things to the table that MOND lacks: (1) a plausible way to generalize it to galaxy cluster phenomena (including the Bullet cluster), (2) an explanation of all or more dark energy phenomena that conserves mass-energy both locally and globally, (3) a plausible means to reconcile the Hubble constant tension, (4) a theoretical framework from which to derive the exact form of the MOND interpolation function and its other conclusions, and (5) one fewer degree of freedom than GR with a cosmological constant, two fewer degrees of freedom than MOND without dark energy or the bare LambdaCDM theory with a single type of sterile dark matter, and three fewer degrees of freedom than MOND with dark energy or LambdaCDM theory with self-interacting dark matter or a fifth DM-baryonic matter force.
If the observationally fitted parameter of Deur's scalar simplification of the GR Lagrangian can't be derived from Newton's constant and geometry and scale, then Deur's theory isn't just a reformulation of Einstein's GR. This would also mean that Deur's approach has the same number of degrees of freedom as GR with a cosmological constant, but it still superior to Lambda-CDM with a single kind of sterile dark matter, in terms of Occam's Razor.
But, if, in fact, Deur's approach is a GR modification rather than true GR (something that can perhaps be described as a quantum gravity effect), for reasons that he failed to appreciate and which critics discerned, this doesn't detract from the fact that:
(1) Deur's approach correctly models systems that LambdaCDM gets wrong observationally,
(2) this approach correctly models systems that MOND gets wrong. observationally,
(3) this approach makes a couple of novel predictions not found in any other prior theory which are confirmed by observations,
(4) this approach has no circumstances where it fails to conform to observational tests and reproduces all of the successes of MOND and of dark matter particle theories, and
(5) integrates all of its conclusions into a theoretical framework with overwhelmingly vanilla theoretical assumptions and just one experimentally measured parameter other than Newton's constant, which has already been determined at the percent level of precision (which is comparable to or better than a number of experimentally measured parameters of the Standard Model and to the cosmological constant of GR and much better than the wildly unconstrained parameter space for dark matter particle theories).
Deur's approach would still be the only theory of dark matter and dark energy phenomena with an unlimited domain of applicability, which makes it an extremely notable theory, even if it turns out that it is actually, contrary to Deur's claims, a modification of GR.
There are also at least a couple of observational tests imminently teed up to compare Deur's predictions to MOND in galaxy scale systems as opposed to the galaxy clusters where Deur already outperfoms MOND: one is the behavior of bodies outside the galactic plane of spiral galaxies (preliminary data favors Deur on this point), and another is the behavior of wide binary systems that are not subject to an external field effect (preliminary data is mixed for this test).
PAllen said:
Deur derives equations by analogies that he never actually derives from GR equations. Thus, I claim Deur is actually a modification of GR. The approximations used have nothing to do with it.
Deur takes two distinct approaches to reach the same result, at least in the limited case of spiral galaxies.
One is to use the GR Lagrangian which is equivalent to Einstein's equations but states those equations in a different form.
Starting from the settled GR Lagrangian, in practice, he then uses a scalar approximation of the GR Lagrangian, which is equivalent to saying that he disregards the elements of the GR stress-energy tensor on the RHS of Einstein's equations other than rest mass (e.g. electromagnetic flux, angular momentum, linear momentum, pressure) which is the same simplifying approximation made when using a Newtonian approximation of GR, and Deur is using this scalar approximation of the GR Lagrangian only in the same circumstances that the Newtonian approximation of GR is used.
For purposes of galaxy and galaxy cluster scale systems, this seems to be a reasonable approximation because there is little interstellar electromagnetic flux (so you can look at the bending of photons by gravity without accounting for the curvature of space flowing from the photons themselves without meaningful loss of accuracy), and because the momentums typical for a galaxy system are much smaller than the speed of light and a zero pressure approximation is common in astronomy systems like these. But, in general, this approximation is not valid in circumstances such as neutron stars, close binary systems, particles moving at relativistic speeds, and magnetars, where full GR and not a scalar approximation of it is needed.
What Deur is not neglecting, however, which conventional GR applications for astronomy in these kinds of systems would, is the non-linearities on the LHS of Einstein's equations that reflect gravitational field self-interaction, which he sometimes calculates with non-perturbative lattice methods.
The new paper reviewing his work argues, although not with complete conviction, that their effort to do the same thing resulted in deviations from Newtonian gravity that are qualitatively similar to those of Deur, but quantitatively much smaller.
The most obvious candidate for the discrepancy is that the self-interaction term of the GR Lagrangian includes a physical constant that should in principle be determinable from first principles in GR using only Newton's constant G and the geometry of the mass distribution. Deur doesn't actually calculate this constant from first principles in GR, however. Instead, he uses the same observations used to establish the MOND critical acceleration a
0 to calibrate this constant in the case of mass distributions with a geometry in line with an idealized spiral galaxy. He basically has faith that the physical constant in question could be calculated and would reproduce the observed value, without actually doing that involved calculation and no later paper from Deur has attempted to do that calculation.
As best I can discern, however, the paper reviewing Deur's work, basically does appear to use first principles to establish the value of this physical constant and in doing so finds that the effect is to small.
My analysis above of what I surmise is going on involves some guesswork and reading between the lines because the paper critical of Deur's approach basically reconstructs its own scalar approximation from scratch and compares its end results with Deur's, rather than going step by step through the analysis that Deur did in order to pinpoint where they believe he veered off course. It could be that this is not actually the issue, but it seems like the point of Deur's analysis most prone to a magnitude of conventional GR self-interaction effect outcome.
If I am right about what is going on, then the basic issue is that Deur is implicitly modifying GR by assuming a stronger coupling between gravitons of a given mass-energy than the coupling between gravitons and other fundamental particles from the Standard Model. (I'd be particularly curious if the strength of the attraction between gravitons was implicitly the square of the naive expectation, but I don't know how the observationally estimated parameter and the first principles parameter compare to each other.)
Another possible source of the discrepancy is that paper reviewing Deur's work is not adequately modeling the system's geometry and overall mass scale correctly, because it fails to appreciate the central importance of these factors.
One problem with simply claiming that Deur's scalar version of the GR Lagrangian approach is wrong, however, is that Deur has replicated the result for spiral galaxies by another independent method that more directly flows from Einstein's equations, rather than from a scalar approximation of the GR Lagrangian.
The other approach used by Deur, although only in a single published paper, is to use a mean field approximation of more conventional classical GR rather than the QCD inspired GR Lagrangian approach. It doesn't appear that the paper critiquing his body of gravitation work considered the approach of that paper.
So, for Deur's analysis to be wrong, both approaches need to have basically the same flaw for different reasons in the specific analysis done in each case.