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We make use of the phase space density approach to discuss gravitino as a warm dark matter candidate. Barring fine tuning between the reheat temperature in the Universe and superparticle masses, we find that \emph{warm} gravitinos have both…

High Energy Physics - Phenomenology · Physics 2009-02-09 D. Gorbunov , A. Khmelnitsky , V. Rubakov

We consider the possibility that supersymmetry is broken above the inflationary mass scale and that the only "low" energy remnant of supersymmetry is the gravitino with mass of order the EeV scale. The gravitino in this class of models…

High Energy Physics - Phenomenology · Physics 2017-08-09 Emilian Dudas , Yann Mambrini , Keith Olive

The axino and the gravitino are extremely weakly interacting candidates for the lightest supersymmetric particle (LSP). We demonstrate that either of them could provide the right amount of cold dark matter. Assuming that a charged slepton…

High Energy Physics - Phenomenology · Physics 2007-05-23 Frank Daniel Steffen

We consider heavy stable neutral particles in the context of supergravity and show that a gravitationally suppressed inflaton decay can produce such particles in cosmologically interesting abundances within a wide mass range $10^3 {\rm GeV}…

High Energy Physics - Phenomenology · Physics 2009-07-07 Rouzbeh Allahverdi , Kari Enqvist , Anupam Mazumdar

Stable particle dark matter may well originate during the decay of long-lived relic particles, as recently extensively examined in the cases of the axino, gravitino, and higher-dimensional Kaluza-Klein (KK) graviton. It is shown that in…

Astrophysics · Physics 2009-11-13 Karsten Jedamzik , Martin Lemoine , Gilbert Moultaka

Gravitino production and decay in the inflationary universe are reexamined. Assuming that the gravitino mainly decays into a photon and a photino, we calculate the upperbound on the reheating temperature. Compared to previous works, we have…

High Energy Physics - Phenomenology · Physics 2017-02-01 M. Kawasaki , T. Moroi

The identity of dark matter is one of the greatest puzzles of our Universe. Its solution may be associated with supersymmetry which is a fundamental space-time symmetry that has not been verified experimentally so far. In many…

High Energy Physics - Phenomenology · Physics 2007-08-28 Frank Daniel Steffen

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

The presence of high reheating temperatures in the thermal history of the universe challenges supersymmetric scenarios owing to the gravitino problem. We revise a general R-parity conserving gravitino dark matter scenario with a stau as the…

High Energy Physics - Phenomenology · Physics 2014-05-26 Jan Heisig

The flux of electron and positron cosmic rays measured by the space-based experiments PAMELA, AMS-02, CALET, DAMPE and Fermi-LAT shows an unexpected behaviour at high energies, in comparison with expectations from standard astrophysical…

High Energy Physics - Phenomenology · Physics 2020-11-19 Johannes Buchner , Edson Carquin , Marco A. Díaz , Germán A. Gómez-Vargas , Boris Panes , Nicolás Viaux

If dark matter possesses a lepton number, it is natural to expect the dark-matter annihilation and/or decay mainly produces the standard model leptons, while negligible amount of the antiproton is produced. To illustrate such a simple idea,…

High Energy Physics - Phenomenology · Physics 2009-03-04 Chuan-Ren Chen , Fuminobu Takahashi

It is shown that the antiproton spectrum reported by the AMS02 collaboration can be accounted for by dark matter (DM) decay if the residence time in the Galactic halo is of order 90 Myr. The DM lifetime assumed, $ 5 \cdot 10^{27}$ s for DM…

High Energy Astrophysical Phenomena · Physics 2018-07-27 David Eichler , Raz Idan , Eyal Gavish , Tanguy Pierog

We find that the quantum of gravity, the graviton, has time-varying mass (the gomidium), and radius (the somium); both vary with the inverse of R; and its frequency is given by Hubble's parameter. Dark matter can be made of such gravitons.…

General Physics · Physics 2012-11-08 Marcelo Samuel Berman

A sufficiently long lived warm dark matter could be a source of X-rays observed by satellite based X-ray telescopes. We consider axinos and gravitinos with masses between 1 keV and 100 keV in supersymmetric models with small R-parity…

High Energy Physics - Phenomenology · Physics 2012-06-01 Paramita Dey , Biswarup Mukhopadhyaya , Sourov Roy , Sudhir K. Vempati

The axino with mass in the GeV region can be cold dark matter(CDM) in the galactic halo. However, if R-parity is broken, for example by the bilinear terms $\mu_\alpha$, then axino($\tilde a$) can decay to $\nu+\gamma$. In this case, the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hang-Bae Kim , Jihn E. Kim

We describe a novel way to measure the mass of heavy, long-lived neutral particles that decay to photons using collider experiments. We focus on a Light Neutralino and Gravitino model in a Gauge Mediated Supersymmetry Breaking scenario…

High Energy Physics - Phenomenology · Physics 2013-09-13 Ziqing Hong , David Toback

It is entirely possible that our Universe is filled with dark radiation, such as SM neutrinos or new physics states, that are sourced by the decay of dark matter with cosmologically long lifetime. If non-thermal neutrinos produced such way…

High Energy Physics - Phenomenology · Physics 2018-12-24 Josef Pradler

It is shown that a decaying neutralino in a supergravity unified framework is a viable candidate for dark matter. Such a situation arises in the presence of a hidden sector with ultraweak couplings to the visible sector where the neutralino…

High Energy Physics - Phenomenology · Physics 2021-08-18 Amin Aboubrahim , Tarek Ibrahim , Michael Klasen , Pran Nath

We present a short review of the status of the dark matter problem. In particular we show that one of the best motivated candidate for the dark matter is the neutralino, a supersymmetric particle. Finally we study the possibility to detect…

Astrophysics · Physics 2007-05-23 Andrea Lionetto

The production and the final abundance of gravitino dark matter appear to depend crucially on the restoration of the global U(1) $R$-symmetry of GMSB sectors in a threefold way. An $R$-symmetric phase effectively suppresses the production…

High Energy Physics - Phenomenology · Physics 2015-06-15 Iannis Dalianis
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