0000000000052124

AUTHOR

Masafumi Koike

showing 5 related works from this author

Big-bang nucleosynthesis and the relic abundance of dark matter in a stau-neutralino coannihilation scenario

2008

A scenario of the Big-Bang Nucleosynthesis is analyzed within the Minimal Supersymmetric Standard Model which is consistent with a stau-neutralino coannihilation scenario to explain the relic abundance of dark matter. We find that we can account for the possible descrepancy of the abundance of $\mathrm{^{7}Li}$ between the observation and the prediction of the Big-Bang Nucleosynthesis by taking the mass of the neutralino as $300 \mathrm{GeV}$ and the mass difference between the stau and the neutralino as $(100 -- 120) MeV$. We can therefore simultaneously explain the abundance of the dark matter and that of $\mathrm{^{7}Li}$ by these values of parameters. The lifetime of staus in this scena…

PhysicsNuclear and High Energy PhysicsParticle physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyDark matterFOS: Physical sciencesSupersymmetryAstrophysicsStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisNucleosynthesisNeutralinoAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentLight dark matterAstrophysics::Galaxy AstrophysicsMinimal Supersymmetric Standard ModelPhysical Review D
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Stau relic density at the big-bang nucleosynthesis era in the coannihilation scenario and a solution to theLi7problem

2010

The work of K. K. was supported in part by PPARC Grant No. PP/D000394/1, EU Grant No. MRTN-CT-2006-035863, the European Union through the Marie Curie Research and Training Network "UniverseNet," MRTN-CT-2006-035863, and Grant-in-Aid for Scientific research from the Ministry of Education, Science, Sports, and Culture, Japan (No. 18071001). The work of M. K. was supported in part by the Grant-in-Aid for the Ministry of Education, Culture, Sports, Science, and Technology, Government of Japan (No. 22740140). The work of J. S. was supported in part by the Grant-in-Aid for the Ministry of Education, Culture, Sports, Science, and Technology, Government of Japan (Nos. 20025001, 20039001, and 205402…

PhysicsNuclear and High Energy PhysicsGovernmentParticle physicsWork (electrical)media_common.cataloged_instanceChristian ministryEuropean unionPublic administrationmedia_commonMarie curiePhysical Review D
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Model building by coset space dimensional reduction in ten dimensions with direct product gauge symmetry

2009

14 pages.-- ISI article identifier:000264762400083.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0812.0910

PhysicsNuclear and High Energy PhysicsScalar (mathematics)High Energy Physics::PhenomenologyYukawa potentialLie groupFOS: Physical sciencesCombinatoricsHigh Energy Physics::TheoryHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Gauge groupQuantum electrodynamicsCosetGauge theoryDirect productGauge symmetry
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GAUGE-HIGGS UNIFICATION MODELS WITH COSET SPACE DIMENSIONAL REDUCTION SCHEME

2009

We investigate the gauge-Higgs unification models within the scheme of the coset space dimensional reduction, beginning with two types of set up; fourteen-dimensional gauge theory with simple gauge groups and ten-dimensional gauge theory with direct product gauge groups. We found some phenomenologically acceptable models through an exhaustive search for the candidates of the coset spaces, the gauge group in higher dimension, and fermion representation.

PhysicsNuclear and High Energy PhysicsIntroduction to gauge theoryQuantum gauge theoryHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAtomic and Molecular Physics and OpticsBRST quantizationHigh Energy Physics::TheoryTheoretical physicsHamiltonian lattice gauge theorySupersymmetric gauge theoryLattice gauge theoryQuantum electrodynamicsGauge anomalyGauge symmetryInternational Journal of Modern Physics A
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Cosmological promising parameters of stau in the minimal supersymmetric standard model

2009

We find that we can account for the possible descrepancy of the primordial abundance of 7 Li between the observation and the prediction of the Big-Bang Nucleosynthesis in a scenario of the Big-Bang Nucleosynthesis with the Minimal Supersymmetric Standard Model. This scenario is consistent with a stau-neutralino coannihilation scenario to explain the relic abundance of dark matter. The solution to the discrepancy is given by taking the values of parameters; the mass of the neutralino as 300 GeV and the mass difference between the stau and the neutralino as (100 – 120) MeV.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsNucleosynthesisHigh Energy Physics::PhenomenologyNeutralinoDark matterHigh Energy Physics::ExperimentAstronomy and AstrophysicsAstrophysics::Galaxy AstrophysicsAtomic and Molecular Physics and OpticsMinimal Supersymmetric Standard Model
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