Particle physics and cosmology
After 1965 Sakharov returned to
fundamental science and began working on
particle physics and
physical cosmology.
[18] [19] [20] [21] [22] [23] [24] [25] [26] [27][28][29][30][31][32]
2D didactic image of Sakharov's model of the universe with reversal of the arrow of time
He tried to explain the
baryon asymmetry of the universe; in that regard, he was the first to give a theoretical motivation for
proton decay. Proton decay was suggested by Wigner in 1949 and 1952.
[33]
Proton decay experiments had been performed since 1954 already.
[34] Sakharov was the first to consider
CPT-symmetric events occurring
before the
Big Bang:
We can visualize that neutral spinless maximons (or photons) are produced at ''t'' < 0 from contracting matter having an excess of antiquarks, that they pass "one through the other" at the instant ''t'' = 0 when the density is infinite, and decay with an excess of quarks when ''t'' > 0, realizing total CPT symmetry of the universe. All the phenomena at t < 0 are assumed in this hypothesis to be CPT reflections of the phenomena at t > 0.
[20]
His legacy in this domain are the famous
conditions named after him:
[20] Baryon number violation, C-symmetry and CP-symmetry violation, and interactions out of thermal equilibrium.
Sakharov was also interested in explaining why the curvature of the universe is so small. This lead him to consider cyclic models, where the universe oscillates between contraction and expansion phases.
[30][29] In those models, after a certain number of cycles the curvature naturally becomes infinite even if it had not started this way: Sakharov considered three starting points, a flat universe with a slightly negative cosmological constant, a universe with a positive curvature and a zero cosmological constant, and a universe with a negative curvature and a slightly negative cosmological constant. Those last two models feature what Sakharov calls a reversal of the time arrow, which can be summarized as follows: He considers times t > 0 after the initial Big Bang singularity at t = 0 (which he calls "Friedman singularity" and denotes Φ) as well as times t < 0 before that singularity. He then assumes that entropy increases when time increases for t > 0 as well as when time decreases for t < 0, which constitutes his reversal of time. Then he considers the case when the universe at t < 0 is the image of the universe at t > 0 under CPT symmetry but also the case when it is not so: the universe has a non-zero CPT charge at t = 0 in this case. Sakharov considers a variant of this model where the reversal of the time arrow occurs at a point of maximum entropy instead of happening at the singularity. In those models there is no dynamic interaction between the universe at t < 0 and t > 0.
In his first model the two universes did not interact, except via local matter accumulation whose density and pressure become high enough to connect the two sheets through a bridge without spacetime between them, but with a continuity of geodesics beyond the Schwarzschild radius with no singularity[
citation needed], allowing an exchange of matter between the two conjugated sheets, based on an idea after
Igor Dmitriyevich Novikov.
[35] Novikov called such singularities a
collapse and an
anticollapse, which are an alternative to the couple
black hole and
white hole in the
wormhole model. Sakharov also proposed the idea of
induced gravity as an alternative theory of
quantum gravity.
[36]
