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Related papers: Neutralino dark matter from heavy axino decay

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Dark-matter particles like neutralinos should decouple from the hot cosmic plasma at temperatures of about 40 GeV. Later they can annihilate each other into standard-model particles, which are injected into the dense primordial plasma and…

High Energy Astrophysical Phenomena · Physics 2016-11-30 Igor N. Mishustin

We review the main proposals of particle physics for the composition of the cold dark matter in the universe. Strong axion contribution to cold dark matter is not favored if the Peccei-Quinn field emerges with non-zero value at the end of…

High Energy Physics - Phenomenology · Physics 2011-01-27 George Lazarides

Moduli, modulini and the gravitino have gravitational-strength interactions, and thermal collisions after reheating create all of them with roughly the same abundance. With their mass of order $100\GeV$, corresponding to gravity-mediated…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H. Lyth

We perform a systematic analysis of dark matter production during post-inflationary reheating. Following the period of exponential expansion, the inflaton begins a period of damped oscillations as it decays. These oscillations and the…

High Energy Physics - Phenomenology · Physics 2020-07-01 Marcos A. G. Garcia , Kunio Kaneta , Yann Mambrini , Keith A. Olive

Cosmological issues are examined when gravitino is the lightest superparticle (LSP) and R-parity is broken. Decays of the next lightest superparticles occur rapidly via R-parity violating interaction, and thus they do not upset the big-bang…

High Energy Physics - Phenomenology · Physics 2011-05-05 Fumihiro Takayama , Masahiro Yamaguchi

In gravity mediated models and in particular in models with strongly stabilized moduli, there is a natural hierarchy between gaugino masses, the gravitino mass and moduli masses: $m_{1/2} \ll m_{3/2} \ll m_{\phi}$. Given this hierarchy, we…

High Energy Physics - Phenomenology · Physics 2015-06-17 Jason L. Evans , Marcos A. G. Garcia , Keith A. Olive

We reconsider post-inflation gravitino production, in the context of hidden sector supergravity models. We discuss the possible role of supersymmetry breaking from finite temperature effects in enhancing the rate for gravitino production…

High Energy Physics - Phenomenology · Physics 2009-10-28 Robert G. Leigh , Riccardo Rattazzi

Solar, atmospheric and reactor neutrino experiments established that neutrinos are massive. It is quite natural then to consider neutrinos as candidate particles for explaining the dark matter in halos around galaxies. We study the…

High Energy Physics - Phenomenology · Physics 2015-06-04 A. Nicolaidis

Axion/axino dark matter (DM) is explored in the minimal supergravity (mSUGRA) and Yukawa-unified supersymmetric grand-unified theory (SUSY GUT) models with surprising results. For this type of scenario, relic DM abundance has three…

High Energy Physics - Phenomenology · Physics 2015-05-14 Heaya Ann Summy

A kinetic mixing between the axion and the inflaton allows for a production of axion dark matter even if the inflationary Hubble scale is smaller than the zero-temperature axion mass. We analyze the axion dynamics in this recently…

High Energy Physics - Phenomenology · Physics 2020-09-10 Takeshi Kobayashi , Lorenzo Ubaldi

In supersymmetric models extended with an anomalous $U(1)_H$ different R-parity violating couplings can yield an unstable neutralino. We show that in this context astrophysical and cosmological constraints on neutralino decaying dark matter…

High Energy Physics - Phenomenology · Physics 2009-09-24 D. Aristizabal Sierra , Diego Restrepo , Oscar Zapata

In split-supersymmetry (split-SUSY), gluino is a metastable particle and thus can freeze out in the early universe. The late decay of such a long-life gluino into the lightest supersymmetric particle (LSP) may provide much of the cosmic…

High Energy Physics - Phenomenology · Physics 2009-11-11 Fei Wang , Wenyu Wang , Jin Min Yang

Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivated dark matter (DM) candidates, whose experimental evidences are very distinctive and different from other standard candidates, as thermal…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. A. R. Cembranos , Jonathan L. Feng , A. Rajaraman , F. Takayama

We consider a class of late-decaying dark-matter models, in which a dark matter particle decays to a heavy stable daughter of approximately the same mass, together with one or more relativistic particles which carry away only a small…

High Energy Astrophysical Phenomena · Physics 2011-12-19 Nicole F. Bell , Ahmad J. Galea , Kalliopi Petraki

Extremely weakly interacting particles like the gravitino may be stable enough on cosmological time scales to constitute a good dark matter candidate even in the presence of R-parity violation. We consider the possibility that the recently…

High Energy Physics - Phenomenology · Physics 2014-07-23 N. -E. Bomark , L. Roszkowski

Supersymmetry breaking sectors generically have an approximate global U(1) $R$-symmetry. Thermal effects tend to restore the $R$-symmetry in the reheated early universe. We revisit the gravitino generation from the thermal plasma and we…

High Energy Physics - Phenomenology · Physics 2013-05-30 Ioannis Dalianis

We re-investigate the evolution of the strongly degenerate neutrinos in the early universe. With the larger degeneracy, the neutrino number freezes at higher temperatures because the neutrino annihilation rate decreases. We consider very…

Astrophysics · Physics 2009-11-07 Kazuhide Ichikawa , M. Kawasaki

We have shown that inflatons with a mass which is calculated to be of the order of $10^{10}\GeV$ can constitute a dominant part of dark matter. They can decay uniquely into a neutrino and antineutrino with a lifetime calculated to be…

Astrophysics · Physics 2007-05-23 Saul Barshay , Georg Kreyerhoff

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…

General Physics · Physics 2014-11-18 A. W. Beckwith

A small breaking of R-parity reconciles thermal leptogenesis, gravitino dark matter and primordial nucleosynthesis. We find that the same breaking relaxes cosmological bounds on the axion multiplet. Naturally expected spectra become allowed…

High Energy Physics - Phenomenology · Physics 2015-05-27 Jasper Hasenkamp , Jörn Kersten
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