Entropy, neutrino physics, and the lithium problem—why stars with no lithium in early universe exist

نویسنده

  • Andrew Beckwith
چکیده

We review how graviton initial energy values are linkable to possible order of the Lorentz gravitational violation. Counter intuitively, the greatest Lorentz gravitational violation would be at lower to moderate initial velocity value conditions due to pre inflationary conditions. .We assume with rapid build up of graviton energies , convergence to flat space, Lorentz invariance as gravitons , due to a high level of initially extreme inflationary conditions speed up with introduction of massively boosted energies at the onset of the big bang.. The coupling of neutrinos to gravitions would be enhanced as their wave lengths would initially be quite similar, i.e. very short.. Consequences for the Lithium problem in stars, due to stellar formation, and gravitational perturbation on DM and will be discussed toward the end of this document. The neutrino / gravitational wave interaction leads to a damping factor in the intensity of GW of ( ) [ ] ( ) [ ] 2 5 1 ρ ρ θ ρ ρ neutrino neutrino + ⋅ − as far as relic GW as could be shown up in the CMBR data sets. This would have no bearing upon the peak of the frequency range, which is another matter entirely. The contention advanced, though is that proper analysis of the big bang, including initial treatment of nucleosynthesis may show a way forward to explain the recent discovery of early old stars with no lithium. Thereby closing one of the huge holes in the big bang, and lithium abundance. Introduction Following a presentation as given for the Gravity Research foundation award essay by Alejandro Jenkens, 2009, the author makes the same dimensional identification that of energy, and energy variation as carried by a graviton μ ⋅ L p ~ 0 and μ ⋅ Δ L E ~ as a way to show how gravitons are linkable to possible order of the Lorentz gravitational Lorentz violation. Note that c v c L ) ( ~ − for the degree of Lorentz violation which involve gravitons with a dispersion relationship of p v E ⋅ ≡ , where v is a speed of propagation of the graviton. Note that the linkage of dispersion relationships of the graviton specifically are linked to a non relativistic treatment of the graviton. Also, left unsaid as a variance is how the strength of the energy interaction,μ , as brought up is linkable to L M Planck ~ μ , where the graviton is to first order an emergent field Goldstone boson. Note that 0 ≠ L is for extension of physics, beyond the standard Model, whereas the standard model has 0 mod tan ⎯ ⎯ ⎯ ⎯ ⎯ ⎯ ⎯ ⎯ ⎯ ⎯ → ⎯ − − − − physics el dard s to approach L . This de couples the graviton, as an emergent boson particle, and has consequences for large scale entropy generation at ultra high speeds, and neutrino physics, and solutions for the entropy problem. L M Planck ~ μ going to zero seems to be inevitable for early universe Graviton physics, with consequences for neutrino physics, unless the graviton is, in this case an emergent ‘wave particle’ entity at intermediate energy regimes, just before the onset of inflation. Most likely, L M Planck ~ μ went to zero, very quickly, or close enough to it, leading to interaction between initial gravitons, and neutrinos , in accordance to Bashinsky’s (2005) analysis that there is a coupling of neutrino and graviton evolutionary radiation era as of the radiation era, due to an increase in the complexity of what would other wise be a simple elaboration of the standard neutrinoless radiation era result , due to no neutrino anisotropic stress . However, graviton waves appear to be partly damped in absolute magnitude , in the in initial inflation to radiation era. Furthermore, as the author will elaborate upon, the lithium problem in early cosmology may be resolvable by explaining how and why

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تاریخ انتشار 2009