MG12 - Talk detail
 

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Abstract

Gravitinos, the Lithium problem, and DM production: Is there a corresponding neutrino physics linkage?

Studies are cited indicating that gravitino production acts as a natural upper bound to Li6 and Li7 levels, based on what happens after hadronic decay of relic 1 TeV into 100 GeV gravitinos at 1000 s. after the Big Bang. The produced gravitinos contribute a large fraction of required dark matter density. Whether or not gravitinos can be linked to neutrino production depends on which model of dark matter (DM) is assumed or used

Entropy growth in the early universe and confirmation of initial big bang conditions

This paper shows how increased entropy values from an initially low big bang level can be measured experimentally by counting relic gravitons. Furthermore the physical mechanism of this entropy increase is explained via analogies with early-universe phase transitions. The role of Jack Ng’s revised infinite quantum statistics in the physics of gravitational wave detection is acknowledged. Ng’s infinite quantum statistics can be used to show that a relic conditions (entropy variation)~ ( particle [gravitons] variation ) is a starting point to the increasing net universe cosmological entropy. Finally, in a nod to similarities with ZPE analysis, it is important to note that the resulting (entropy variation)~ ( particle [gravitons] variation ) is much less than 10 to the 88 power , that in fact it is much lower, allowing for evaluating initial graviton production as an emergent field phenomena, which may be similar to how ZPE states can be used to extract energy from a vacuum if entropy is not maximized. The rapid increase in entropy so alluded to without near sudden increases to 10 to the 88 power may be enough to allow successful modeling of relic graviton production for entropy in a manner similar to ZPE energy extraction from a vacuum state. I.e. avoiding maximization of entropy, so energy extraction from a vacuum state may commence, as an emergent field phenomena, in the initial states of inflation.

Stretched neutrinos, and the supposed linkage to Gravitons/ HFGW data sets

Following discussion of George Fuller and Chad Kishimoto, in PRL, 2009, the issue of if or not a correlation exist between neutrino physics, and HFGW data sets / gravitons will be raised anew, with a particular emphasis upon what happens if the following scenario outlined by Fuller and Kishimoto arises. What if as the “universe expanded, the most massive of these states slowed down in the relic neutrinos, stretching them across the universe”. If an initial close correlation between Gravition data sets/ HFGW and relic neutrinos exists in the beginning, do we have in any case a situation where there is a corresponding ‘stretch out’ of gravitons? If so, what would this say about the relevant requirements for graviton/ HFGW detectors?

Stretched neutrinos, and the supposed linkage to Gravitons/ HFGW data sets

Following discussion of George Fuller and Chad Kishimoto, in PRL, 2009, the issue of if or not a correlation exist between neutrino physics, and HFGW data sets / gravitons will be raised anew, with a particular emphasis upon what happens if the following scenario outlined by Fuller and Kishimoto arises. What if as the "universe expanded, the most massive of these states slowed down in the relic neutrinos, stretching them across the universe". If an initial close correlation between Gravition data sets/ HFGW and relic neutrinos exists in the beginning, do we have in any case a situation where there is a corresponding 'stretch out' of gravitons? If so, what would this say about the relevant requirements for graviton/ HFGW detectors?

Gravitinos, the Lithium problem, and DM production: Is there a corresponding neutrino physics linkage?

Studies are cited indicating that gravitino production acts as a natural upper bound to Li6 and Li7 levels, based on what happens after hadronic decay of relic 1 TeV into 100 GeV gravitinos at 1000 s. after the Big Bang. The produced gravitinos contribute a large fraction of required dark matter density. Whether or not gravitinos can be linked to neutrino production depends on which model of dark matter (DM) is assumed or used

Entropy growth in the early universe and confirmation of initial big bang conditions, via quantum cosmology

This paper shows how increased entropy values from an initially low big bang level can be measured experimentally by counting relic gravitons. Furthermore the physical mechanism of this entropy increase is explained via analogies with early-universe quantum phase transitions. The role of Jack Ng’s revised infinite quantum statistics in the physics of gravitational wave detection is acknowledged. Ng’s infinite quantum statistics can be used to show that [change in entropy ] is proportional to [cnange in the number of gravitons] is a starting point to the increasing net universe cosmological entropy. Finally, in a nod to similarities with ZPE analysis, it is important to note that the resulting change in relic graviton number must be not equal to 10 to the 88 power , that in fact it is much lower, allowing for evaluating initial graviton production as an emergent field phenomena, which may be similar to how ZPE states can be used to extract energy from a vacuum if entropy is not maximized. The rapid increase in entropy so alluded to without near sudden increases to 10 to the 88 power may be enough to allow successful modeling of relic graviton production for entropy in initial states is a quantum cosmological in a manner similar to ZPE energy extraction from a vacuum state.

Can quantum infinite statistics as presented by Jack Ng specify a linkage between gravitons/gravitinos, and Dark Matter?

As of 2007 , and recently in 2008, Jack Ng in ,” Quantum Foam and Dark Energy”, International work shop on the Dark Side of the Universe" specified a particle counting algorithm, as derived from quantum 'infinite' statistics for increases in entropy which, the author asserts for certain spatial regimes ( on the order of , or greater than Planck Length) which would mandate high frequency gravitational waves. Ng's supposition was that long range spatial regimes as part of a modified partition function would lead to interesting DM candidates. The talk specifies certain thought experiments which, upon elaboration of quantum geometry may lead to a correspondence between Dark matter and certain types of gravitino candidates, which are then linked to gravitons via dimensional scaling arguments. This adds additional definition to typical SUSY treatments of DM/ gravitinos, and is a short hand way of relating SUSY partners to their non SUSY counter parts in early universe General relativity

Comparison of DM, Gravitons, and Entropy generation in relic conditions. Is Quantum foam a candidate for linkage?

The author ,(following Y. Jack. Ng in his explicit derivation of a counting algorithm of relating an increase in entropy due to a change in particle count as obtained via use of ‘infinite quantum statistics’ as can be seen from his article ” Space time Foam: From Entropy and Holography to Infinite Statistics and Nonlocality” Entropy 2008), asks if there is an explicit linkage between gravitinos,DM,and early synthesis of gravitons in relic conditions. The formation of emergent relic ‘particles’ if confirmed via falsifiable procedure may be a proof of the quantum foam hypothesis. In addition , showing relic particle formation, i.e. gravitons may be a way of answering if gravity is due to either an emergent field/ other configurations contributing to the growth of entropy in the onset of inflation.

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