227 research outputs found
Relic High Frequency Gravitational waves from the Big Bang, and How to Detect Them
We show conditions for HFGW detection, employing an entropy concept written
up by Jack Ng, and Steinhard's proceedure for reconstructing tensorial
representations for relic HFGW from the onset of the big bang. The issue of the
reality of gravitons as a measurable physical object which was raised by
Rothman in 2006 is indirectly answered via a proceedure obtained from
Weinberg's 1972 book on gravitation, and all the methodologies so obtained are
referenced with respect to engineering specifications of the Li-Baker HFGW
detector. In addition, the document also refers to entanglement entropy, and
its possible aid in refining measurement predictions. Finally, commentary about
HFGW and relic neutrino physics data sets is included, with regards to
inflationary model candidatesComment: 15 pages, 1 table, 1 figure. Covers two AIP conference proceeding
entries. Pages 1-9 correspond to one ias-spes Huntsville, Alabama February
2009 conference paper on the formalism of HFGW analysis, and pages 9-13
correspond to Neutrino physics-HFGW data set comparison, in terms of
different inflationary potential candidate
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. A model presented by the
author in 2008 links DM of about 100 GeV -- based on a phenomenological
Lagrangian creating different Neutrino masses without SUSY -- with a dark
matter candidate of about 100 GeV. This may tie in 100 GeV gravitinos with
neutrino physics.Comment: 2 pages, no figures. New article in a sequel of DM applications
articles. Conference entry to Rencontres De Moriond, for the Cosmology
meeting, February 2009, to be published late 2009 by the Gioi company of
Vietna
Analyzing Black Hole super-radiance Emission of Particles/Energy from a Black Hole as a Gedankenexperiment to get bounds on the mass of a Graviton
Use of super-radiance in BH physics, so dE/dt < 0 specifies conditions for a
mass of a graviton being less than or equal to 10^ - 65 grams, and also allows
for determing what role additional dimensions may play in removing the datum
that massive gravitons lead to 3/4th the bending of light past the planet
Mercury.The present document makes a given differentiation between
super-radiance in the case of conventional BHs and Braneworld BH
super-radiance, which may delineate if Braneworlds contribute to an admissible
massive graviton in terms of removing the usual problem of the 3/4th the
bending of light past the planet Mercury which is normally associated with
massive gravitons. This leads to a fork in the road, between two alternatives
with the possibility of needing a multiverse containment of BH structure, or
embracing what Hawkings wrote up recently, namely a re do of the Event Horizon
hypothesis as we know it.Comment: 7 pages, research article, Advances in High Energy Physics 201
How To Have a Transfer of Information From a Prior to a Present Universe, in Lieu of Information Theory
What happens to the topological entanglement entropy of a system, when it is driven out of its ground state by increasing the temperature? This question is basic, especially if there is an increasing amount of temperature up to the interval of Planck time, in early universe cosmology. The author examines what is possible if a cyclic model is arranged via Penrose cyclic cosmology, which may enable entanglement entropy as a way to transfer essential information from a prior to the present universe. We reference Theorem 6.1.2 of the book by Ellis, Maartens, and MacCallum in order to argue that if there is a non zero initial scale factor, that there is a partial breakdown of the Fundamental Singularity theorem which is due to the Raychaudhuri equation. Afterwards, we review a construction of what could happen if we put in what Ellis, Maartens, and MacCallum call the measured effective cosmological constant and substitute Effective ïŒ ï‚® ïŒ in the Friedman equation. I.e. there are two ways to look at the problem, i.e. after Effective ïŒ ï‚® ïŒ , set Vac ïŒ as equal to zero, and have the leftover ïŒ as scaled to background cosmological temperature, as was postulated by Park (2002) or else haveVac ïŒ as proportional to ïŒVac ~1038GeV2which then would imply using what we call a 5 dimensional contribution to ïŒ as proportional to 5 ~ const/ T D ï¢ ïŒ ï‚» ïŒ  . We find that both these models do not work for generating an initial singularity. ïŒ removal as a non zero cosmological constant is most easily dealt with by a Bianchi I universe version of the generalized Friedman equation
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