Hence, the plausibility of the causality of Smolin's Autodidactic Universe.The 
Laws of the Universe Are Changing | RealClearScience
Slum-dunk? No, there is only more research to be funded to search for what can 
be detected.
For this peasant? A great working theory.


-----Original Message-----
From: Lawrence Crowell <goldenfieldquaterni...@gmail.com>
To: Everything List <everything-list@googlegroups.com>
Sent: Fri, Dec 30, 2022 10:04 am
Subject: Re: Physics? Ok Astronomers view 2 distant Water Worlds so following 
the physics I ask..

On Wednesday, December 28, 2022 at 11:41:36 PM UTC-6 Bruce wrote:

On Thu, Dec 29, 2022 at 4:34 PM Brent Meeker <meeke...@gmail.com> wrote:

 On 12/28/2022 9:01 PM, Bruce Kellett wrote:
  
   On Thu, Dec 29, 2022 at 3:29 PM Brent Meeker <meeke...@gmail.com> wrote:
    
  Of course one reason there are "laws of physics" is what my late friend Vic 
Stenger called Point Of View Invariance.  This was his generalization of Emmy 
Noether's theorem that showed every symmetry implied a conservation law. 
 
  That is not strictly true. It is only continuous symmetries of the Lagrangian 
that imply conservation laws -- not all symmetries. For example, the symmetries 
of a square under rotation and reflection do not generate any conservation 
laws. Neither do discrete symmetries like parity and charge conjugation. 
  
 So momentum is conserved because we want any law of physics to be invariant 
under translation of a different location.  Energy is conserved because we want 
the laws of physics to be the same at different times, etc. 
 
  It is not what we want, it is what we find. We find that nature is invariant 
under these continuous transformations, so we build those symmetries into our 
laws.   
 
 Vic called in POVI because he wanted to extend it to transformations in 
abstract spaces, e.g. gauge invariance.  Of course the invariance depends on 
the "point of view" in a sense.  Things didn't look at all space translation 
invariant to Aristotle.  Galileo said ignore that your ship is moving along the 
shore, just look at the dynamics in the cabin.  So we discovered these 
symmetries by learning what ignore as well as what to measure.

The real point is that the laws are discovered, not imposed. The fact that 
continuous symmetries correspond to conservation laws was discovered only very 
much later. Most of the history of physics is about discovering what works -- 
what the laws might be. POVI was thought of only very late in the game, and is 
not a fundamental insight.
Bruce

This begins to look a bit similar to the debate over whether mathematics is 
objectively real or something invented.  Emmy Noether gave consideration to 
that boundary term we usually discard when deriving the Euler-Lagrange formula 
to show that a symmetry was involved with this term. This symmetry and that 
this boundary term is zero meant a conservation law. A law of physics 
considered as such is something associated with covariant and invariant 
properties of space, spacetime or an abstract space under some set of 
transformations. Is this principle, a law of laws should we say, something that 
is discovered or is some objective aspect of a mathematical reality?

The type D, II, III and N solutions, black holes = D and gravitational waves = 
N, are vacuum solutions with the Weyl tensor C_{abcd} that wholly determines 
the curvature. The Weyl curvature is an operator on Killing vectors, such that 
Killing vectors are eigenvalued with the Weyl curvature C_{abcd}K^bK^d = 
λK_aK_c. The type N solutions have Killing vectors that have zero eigenvalue 
C_{abcd}K^d = 0. Type III spacetimes have λ = 0 and type II and D have 
nontrivial eigenvalues that are unequal for C_{abcd} and *C_{abcd}, for * the 
Hodge dual with C_{abcd}K^bK^d = λK_aK_c and *C_{abcd}K^bK^d = λ’K_aK_c for λ ≠ 
λ’ and λλ ≠ 0. These Killing vectors define symmetries and thus conservation 
laws. A timelike Killing vector defines conservation of energy, a spacelike 
Killing vector defines conservation of momentum, and a Killing bi-vector or one 
derived from such defines conservation of angular momentum. That is a total of 
1 + 3 + 6 = 10 Killing vectors. These eigenvalued equations should make one 
think of the Schrodinger equation. Indeed for a timelike Killing vector K_t = 
√(g_{tt})∂_t so that this gives a general wave equation HΨ[g] = iK_t∂Ψ[g]/∂t, 
which for g_{tt} = 1 is the Schrodinger equation. The ADM approach to general 
relativity give NH = 0 and the Wheeler-deWitt equation HΨ[g] = 0. General 
relativity does not automatically define conservation laws. Conservation laws 
only occur with certain symmetries of spacetime. This often occurs where there 
is an ADM mass defined by an asymptotic condition of flatness or some other 
spacetime with constant curvature at a distance.

Conservation laws appear as asymptotic or boundary terms. The AdS/CFT 
correspondence of Maldacena shows that a nonlocal quantum gravity theory 
corresponds to a local conformal field theory on the conformal boundary of the 
anti-de Sitter spacetime. The anti-de Sitter (AdS) spacetime has constant 
negative curvature. This is a negative vacuum energy, where this has some 
correspondence with string theory, such as the type I string theory has a 
negative energy vacuum and its first excited state is a negative energy state. 
The AdS_4 has a correspondence with black hole physics. The AdS spacetime is 
not the spacetime of the observable universe. It is though in line with the 
theory of Emmy Noether, also work by Hurzebruch, and even the old Gauss-Bonnet 
theory. 

Physical spacetime is more similar to de Sitter spacetime, and is the 
Friedmann-Lemaitre-Robertson-Walker spacetime with positive energy. This means 
curvature is positive, which involves how space is embedded in spacetime, and 
this does not have conservation laws. If that space is a sphere S^3 the 
constant vacuum energy on this space grows with the evolution of this space and 
volume growth. This is one reason that people tend to prefer the flat space 
model, where vacuum energy is net "infinity" and remains so. However, there is 
nothing to prevent vacuum energy density from changing. The phantom energy 
model leading to a big rip of the cosmos is possible, and the curious 
discrepancy between CMB and SNII data, with the Hubble constant H = 
70km/sec-Mpc and H = 74km/sec-Mpc respectively, appears to resist analysis 
meant to show it is zero. If the phantom energy model should be realized then 
conservation of energy, even with an infinite flat space, is gone.

The expansion of the universe also means we will not be able to observe much 
physics that could be called “pre-cosmic,” or the quantum gravitation of the 
pre-inflationary universe. Because of inflation and this 60-efolds of 
expansion, expansion by ~ 10^{29}, a Planck scale region was expanded from 
10^{-33}cm to 10^{-4} cm. Since inflation began at 10^{30} sec in the early 
universe, any Planck scale fluctuation involved with the generation of the 
universe would have been 10^{-23}cm, and was expanded to 10^6 cm --- beyond the 
scale of the then observable universe ~ 10cm.  After inflation the observable 
universe with a scale of ~ 10cm an possible Planck scale process was stretched 
by more normal expansion to 10^{10} light years, and might appear as some order 
anisotropy in the CMB. Using blackbody physics, these quanta would have been a 
tiny aspect of the early universe. These would be very difficult to find in the 
CMB. Beyond that, we cannot observe anything. Any pre-cosmic physics emerged 
from something smaller than the Planck scale and is expanded beyond any 
measurable scale on the CMB. 

John Wheeler said that the ultimate law of physics is there is no law. We may 
then have something similar to this, where what we call the laws of physics are 
just local emergent pattern in the observable universe. At large the universe 
may simply have no conservation laws and ultimate there are globally no 
physical laws.
LC


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