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We study a leptogenesis via decays of heavy Majorana neutrinos produced non-thermally in inflaton decays. We find that this scenario is fully consistent with existing supersymmetric inflation models such as for topological or for hybrid…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Asaka , K. Hamaguchi , M. Kawasaki , T. Yanagida

The lepton flavour violating charged lepton decays mu to e + gamma and thermal leptogenesis are analysed in the minimal supersymmetric standard model with see-saw mechanism of neutrino mass generation and soft supersymmetry breaking terms…

High Energy Physics - Phenomenology · Physics 2007-05-23 S. T. Petcov , T. Shindou

Thermal leptogenesis is an attractive mechanism for generating the baryon asymmetry of the Universe. However, in supersymmetric models, the parameter space is severely restricted by the gravitino bound on the reheat temperature $T_{RH}$.…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sacha Davidson

We investigate the possibility that right-handed (RH) sneutrinos and gravitinos can coexist and explain the dark matter (DM) problem. We compare extensions of the minimal supersymmetric standard model (MSSM) and the next-to-MSSM (NMSSM)…

High Energy Physics - Phenomenology · Physics 2023-04-28 Jong Soo Kim , Daniel E. Lopez-Fogliani , Andres D. Perez , Roberto Ruiz de Austri

We present a supersymmetric extension of the Standard Model that posseses a continuous $ U(1)_R$ symmetry, which is identified with one of three lepton numbers, and where a sneutrino vev gives mass to the down type quark and leptons. This…

High Energy Physics - Phenomenology · Physics 2013-05-30 Claudia Frugiuele , Thomas Gregoire

We calculate exotic cooling rates of stars due to photo-production of light particles (mostly scalars and pseudoscalars) which originate from the hidden sector of no scale supergravity theories. Using this we can restrict the gravitino mass…

High Energy Physics - Phenomenology · Physics 2009-10-28 M. Nowakowski , S. D. Rindani

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

High Energy Physics - Phenomenology · Physics 2007-06-29 David Gherson

Under general circumstances full thermal equilibrium may not be established for a long period after perturbative or non-perturbative decay of the inflaton has completed. One can instead have a distribution of particles which is in kinetic…

High Energy Physics - Phenomenology · Physics 2007-05-23 Rouzbeh Allahverdi , Anupam Mazumdar

In light of recent 80-137 $\rm{fb}^{-1}$ results at the LHC Run 2 establishing a lower gluino mass limit of 2.25 TeV, we revisit the supersymmetric GUT model Flipped $SU$(5) with extra vector-like particles, known as $\cal{F}$-$SU$(5), with…

High Energy Physics - Phenomenology · Physics 2019-10-25 Thomas Ford , Tianjun Li , James A. Maxin , Dimitri V. Nanopoulos

Under the assumption of hierarchical right-handed neutrino masses, masses of right-handed neutrinos must be larger than $10^8$ GeV in the standard thermal leptogenesis scenario, while the mass can be reduced to around 5 TeV in a…

High Energy Physics - Phenomenology · Physics 2013-08-15 Naoyuki Haba , Osamu Seto , Yuya Yamaguchi

The lightest supersymmetric particles could be higgsinos that have a small mixing with gauginos. If the lightest higgsino-like state makes up some or all of the dark matter with a thermal freezeout density, then its mass must be between…

High Energy Physics - Phenomenology · Physics 2024-05-08 Stephen P. Martin

Thermal dark matter that couples more strongly to electrons and photons than to neutrinos will heat the electron-photon plasma relative to the neutrino background if it becomes nonrelativistic after the neutrinos decouple from the thermal…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Chiu Man Ho , Robert J. Scherrer

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

We develop a string-inspired model for particle cosmology, based on a flipped SU(5)$\times$U(1) gauge group formulated in a no-scale supergravity framework. The model realizes Starobinsky-like inflation, which we assume to be followed by…

High Energy Physics - Phenomenology · Physics 2020-02-05 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive

In this letter we have presented a novel version of "long-lived" gluinos in supersymmetric models with the gluino the lightest ordinary supersymmetric particle [LOSP] and axino LSP. Within certain ranges of the axion decay constant $f_a < 1…

High Energy Physics - Phenomenology · Physics 2015-12-09 Stuart Raby

We revisit the cosmology of the supersymmetric QCD axion, highlighting the existence of a serious cosmological axino problem that is fully analogous to the gravitino problem of overclosure via thermal production. A general analysis implies…

High Energy Physics - Phenomenology · Physics 2015-05-27 Clifford Cheung , Gilly Elor , Lawrence J. Hall

We study models in which the universe exits reheating at temperatures in the MeV regime. By combining light element abundance measurements with cosmic microwave background and large scale structure data we find a fairly robust lower limit…

Astrophysics · Physics 2008-11-26 Steen Hannestad

Since the thermal history of the Universe is unknown before the epoch of primordial nucleosynthesis, the largest temperature of the radiation dominated phase (the reheating temperature) might have been as low as 1 MeV. We perform a…

High Energy Physics - Phenomenology · Physics 2009-11-07 N. Fornengo , A. Riotto , S. Scopel

In the light of recent experimental data on gaugino searches, we revisit the direct-transmission model of dynamical supersymmery breaking with the gravitino mass m_{\tilde{G}}\leq 16 eV, which does not have any cosmological or astrophysical…

High Energy Physics - Phenomenology · Physics 2010-04-05 Masahiro Ibe , Kazuhiro Tobe , Tsutomu Yanagida

Affleck-Dine baryogenesis, accompanied by the formation and subsequent decay of Q-balls, can generate both the baryon asymmetry of the universe and dark matter in the form of gravitinos. The gravitinos from Q-ball decay dominate over the…

High Energy Physics - Phenomenology · Physics 2010-10-27 Ian M. Shoemaker , Alexander Kusenko