English
Related papers

Related papers: Gravitino Freeze-In

200 papers

We study the effects of the unstable gravitino on the big-bang nucleosynthesis. If the gravitino mass is smaller than \sim 10 TeV, primordial gravitinos produced after the inflation are likely to decay after the big-bang nucleosynthesis…

High Energy Physics - Phenomenology · Physics 2008-11-26 Kazunori Kohri , Takeo Moroi , Akira Yotsuyanagi

Effects of the unstable gravitino on the big-bang nucleosynthesis (BBN) and its implications to particle cosmology are discussed. If the gravitino mass is smaller than \sim 20 TeV, lifetime of the gravitino becomes longer than \sim 1sec and…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takeo Moroi

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

Scenarios with gravitino dark matter face potential cosmological problems induced by the presence of the Next-to-Lightest Supersymmetric Particle (NLSP) at the time of Big Bang Nucleosynthesis (BBN). A very simple, albeit radical, solution…

High Energy Physics - Phenomenology · Physics 2007-10-16 Alejandro Ibarra

We investigate the production of neutralino dark matter in a cosmological scenario featuring an early matter dominated era ending at a relatively low reheating temperature. In such scenarios different production mechanisms of weakly…

High Energy Physics - Phenomenology · Physics 2018-12-18 Manuel Drees , Fazlollah Hajkarim

The purely gravitational dark matter (PGDM) which interacts with the standard model particles only by gravitational interaction has recently been discussed. Due to its feeble interaction, PGDM may be produced mainly by the gravitational…

High Energy Physics - Phenomenology · Physics 2019-02-28 Soichiro Hashiba , Jun'ichi Yokoyama

Gravitino is one feasible candidate for the dark matter in supergravity models. With its couplings being suppressed by the Plank mass, gravitino interacts very weakly with other particles, making its direct detection, or production at…

High Energy Physics - Phenomenology · Physics 2007-09-26 Yudi Santoso

If the lightest supersymmetric particle (LSP) is Higgsino-like, the thermal relic density is lower than the observed dark matter content for a LSP mass in the sub-TeV region. We outline constraints arising from the Fermi Gamma-Ray Telescope…

High Energy Physics - Phenomenology · Physics 2013-05-30 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

An unstable gravitino with lifetime longer than $10^{26}$ sec or so has been proposed as a possible dark matter candidate in supergravity models with R-parity breaking. We find a natural realization of this idea in the minimal…

High Energy Physics - Phenomenology · Physics 2010-05-12 Xiangdong Ji , Rabindra N. Mohapatra , Shmuel Nussinov , Yue Zhang

The scenario of gravitino dark matter with broken R-parity naturally reconciles three paradigms that, albeit very well motivated separately, seem to be in mutual conflict: supersymmetric dark matter, thermal leptogenesis and standard Big…

Astrophysics · Physics 2009-06-23 Alejandro Ibarra , David Tran

Starting with the vacuum fluctuation, it is known that gravitinos will be created just after inflation, with number density $\sim 10^{-2}M^3$ where $M$ is the mass of the inflaton. Here, we argue that creation may be expected to continue,…

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

We consider the phenomenological implications of gravitino dark matter in the context of the $\mu\nu$SSM. The latter is an R-parity breaking model which provides a solution to the $\mu$-problem of the MSSM and explains the origin of…

High Energy Physics - Phenomenology · Physics 2009-12-10 Carlos Munoz

If a bosonic partner of a right-handed neutrino dominates the early universe sufficiently before its decay, important ingredients in the present universe are related to physics of the right-handed neutrino sector. In particular, we find…

High Energy Physics - Phenomenology · Physics 2009-11-10 M. Ibe , T. Yanagida

We compute the density of a spin-$\frac32$ particle, the raritron, produced at the end of inflation due to gravitational interactions. We consider a background inflaton condensate as the source of this production, mediated by the exchange…

High Energy Physics - Phenomenology · Physics 2025-10-22 Kunio Kaneta , Wenqi Ke , Yann Mambrini , Keith A. Olive , Sarunas Verner

We conduct a systematic investigation of freeze-in during reheating while taking care to include both direct and indirect production of dark matter (DM) via gravitational portals and inflaton decay. Direct production of DM can occur via…

High Energy Physics - Phenomenology · Physics 2024-12-19 Stephen E. Henrich , Yann Mambrini , Keith A. Olive

Models of leptogenesis are constrained by the low reheat temperature at the end of reheating associated with the gravitino bound. However a detailed view of reheating, in which the maximum temperature during reheating, $\Tmax$, can be…

High Energy Physics - Phenomenology · Physics 2008-11-26 Raghavan Rangarajan , Narendra Sahu

The freeze-in mechanism describes the out-of-equilibrium production of dark matter (DM) particles via feeble couplings or non-renormalisable interactions with large suppression scales. In the latter case, predictions suffer from a strong…

High Energy Physics - Phenomenology · Physics 2025-04-16 Cristina Benso , Felix Kahlhoefer , Henda Mansour

We propose the hybrid gravity-gauge mediated supersymmetry breaking where the gravitino mass is about several GeV. The strong constraints on supersymmetry viable parameter space from the CMS and ATLAS experiments at the LHC can be relaxed…

High Energy Physics - Phenomenology · Physics 2015-06-03 Zhaofeng Kang , Tianjun Li

Standard Big Bang nucleosynthesis at baryonic density as inferred by WMAP implies a primordial Li7 abundance factor of two to three larger than that inferred by observations of low--metallicity halo stars. Recent observations of Li6 in halo…

High Energy Physics - Phenomenology · Physics 2009-11-11 Karsten Jedamzik , Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

Since the first detection of gravitational waves by ground-based interferometers, it has emerged as a novel probe for exploring physics in the early universe. The particle nature of cold dark matter (DM) and its underlying production…

High Energy Physics - Phenomenology · Physics 2025-08-15 Yonghua Wang , Wei Chao