Question AXION GLUON MATTER AS DARK MATTER

[Harry Costas]

Hello Jzz
I try to avoid Dark Matter Dark Energy.
My approach is from compact matter, being condensates.

Transients of Condensates. From Atomic to Neutron matter to quark matter to Axion matter and so on.

Compact core having a common property, Dipolar Electro-Magnetic vector field, created by Chiral Super-Symmetry.
This vector field (Vortex) expels matter away from the core.

Cores such as our Sun, Condensates (BH) center of the Milkyway, Core of M87.

Jzz, its past my bedtime and my brain is half here.

 

[Jzz]

Transients of Condensates. From Atomic to Neutron matter to quark matter to Axion matter and so on.

Compact core having a common property, Dipolar Electro-Magnetic vector field, created by Chiral Super-Symmetry.
This vector field (Vortex) expels matter away from the core.

Cores such as our Sun, Condensates (BH) center of the Milkyway, Core of M87.

Jzz, its past my bedtime and my brain is half here.

No problem , take it easy have a good rest and wake up refreshed. The aether based theory suggested by myself, offers the kind of connectedness that is lacking in quantum mechanics. Beginning with a better explanation for why the electron does not spiral into the nucleus, which in turn automatically negates the use of Schrodinger's equation and wave-functions, the theory offers a complete explanation of nature, which is what physics is supposed to do. I suggest once more, that you go through the link to my paper on "Redefining Electrons: A Modern Theory of the Aether" that I had posted and then, if you have any questions or objections to raise those objections and questions. Which would be a more ordered way to proceed.

 

[Harry Costas]

Aether
Tell me more.

 

[Harry Costas]

If Axion matter played an important role in the early stages, why can't it play a role now.

[Submitted on 23 Aug 2023]

QCD Axion Hybrid Inflation​

Yuma Narita, Fuminobu Takahashi, Wen Yin

When the inflaton is coupled to the gluon Chern-Simons term for successful reheating, mixing between the inflaton and the QCD axion is generally expected given the solution of the strong CP problem by the QCD axion. This is particularly natural if the inflaton is a different, heavier axion. We propose a scenario in which the QCD axion plays the role of the inflaton by mixing with heavy axions. In particular, if the energy scale of inflation is lower than the QCD scale, a hybrid inflation is realized where the QCD axion plays the role of the inflaton in early stages. We perform detailed numerical calculations to take account of the mixing effects. Interestingly, the initial misalignment angle of the QCD axion, which is usually a free parameter, is determined by the inflaton dynamics. It is found to be close to π in simple models. This is the realization of the pi-shift inflation proposed in previous literature, and it shows that QCD axion dark matter and inflation can be closely related. The heavy axion may be probed by future accelerator experiments.