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If the scalar tau $\stau$ is the next lightest supersymmetric particle and decays into a gravitino ($\gravitino$) being the lightest supersymmetric particle, it will have generally a very long lifetime. In this paper, we investigate the…

High Energy Physics - Phenomenology · Physics 2010-10-27 Koichi Hamaguchi , Mihoko M. Nojiri , Albert de Roeck

Comparing Big Bang Nucleosynthesis predictions with the light element abundances inferred from observational data, we can obtain the strong constraints on some neutrino properties, e.g. number of neutrino species, mass, lifetime. Recently…

Astrophysics · Physics 2016-08-30 M. Kawasaki , K. Kohri , Katsuhiko Sato

We demonstrate that megaton-mass neutrino telescopes are able to observe the signal from long-lived particles beyond the Standard Model, in particular the stau, the supersymmetric partner of the tau lepton. Its signature is an excess of…

A number of popular extensions of the Standard Model of particle physics predict the existence of doubly charged scalar particles $X^{\pm\pm}$. Such particles may be long-lived or even stable. If exist, $X^{--}$ could form atomic bound…

High Energy Physics - Phenomenology · Physics 2022-09-15 Evgeny Akhmedov

We present supersymmetric scenarios with gravitino LSP and stau NLSP in the case of a non-standard model of cosmology with the addition of a dark component in the pre-BBN era. In the context of the standard model of cosmology, gravitino LSP…

High Energy Physics - Phenomenology · Physics 2011-03-24 Sean Bailly

Neutrino telescopes may have the potential to detect the quasi-stable staus predicted by supersymmetric models. Detection depends on stau electromagnetic energy loss and weak interactions. We present results for the weak interaction…

High Energy Physics - Phenomenology · Physics 2008-11-26 Yiwen Huang , M. H. Reno , I. Sarcevic , J. Uscinski

We consider SUSY extensions of the standard model where the gravitino is the dark-matter particle and the stau is long lived. If there is a significant mass gap with squarks and gluinos, the staus produced at hadron colliders tend to be…

High Energy Physics - Phenomenology · Physics 2015-06-05 R. Barcelo , J. I. Illana , M. Masip , A. Prado , P. Sanchez-Puertas

A star burns its nuclear fuel and balances gravitation by the pressure of the heated gas, during its active lifetime. After the exhaustion of the nuclear fuel, a low mass star finds peace as a {\em white dwarf}, where the pressure support…

Popular Physics · Physics 2017-09-14 Sushan Konar

Active galactic nuclei and gamma ray bursts at cosmological distances are sources of high-energy electron and muon neutrinos and provide a unique test bench for neutrino instability. The typical lifetime-to-mass ratio one can reach there is…

High Energy Physics - Phenomenology · Physics 2010-12-03 P. Keranen , J. Maalampi , J. T. Peltoniemi

We review a non-standard Big-Bang nucleosynthesis (BBN) scenario within the minimal supersymmetric standard model, and propose an idea to solve both ${}^{7}$Li and ${}^{6}$Li problems. Each problem is a discrepancy between the predicted…

High Energy Physics - Phenomenology · Physics 2017-09-20 Joe Sato , Takashi Shimomura , Masato Yamanaka

Recently, an excess of events consistent with a Higgs boson with mass of about 125 GeV was reported by the CMS and ATLAS experiments. This Higgs boson mass is consistent with the values that may be obtained in minimal supersymmetric…

High Energy Physics - Phenomenology · Physics 2017-08-23 Marcela Carena , Stefania Gori , Nausheen R. Shah , Carlos E. M. Wagner , Lian-Tao Wang

The cosmological relic density of the lightest supersymmetric particle of the minimal supersymmetric standard model is calculated under the assumption of gauge and Yukawa coupling unification. We employ radiative electroweak breaking with…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. E. Gomez , G. Lazarides , C. Pallis

We study the stau lifetime in a scenario with the LSP taken to be a neutralino and the NLSP being a stau, based on the minimal supersymmetric Standard Model. The mass difference between the LSP and NLSP, $\delta m$, must satisfy $\delta…

High Energy Physics - Phenomenology · Physics 2008-11-26 Toshifumi Jittoh , Joe Sato , Takashi Shimomura , Masato Yamanaka

We discuss fluxes of long-lived supersymmetric (SUSY) particles produced in the atmosphere from ultra-high energy cosmic-ray interactions with air nuclei. We consider long-lived particle production which proceeds first via the on-shell…

High Energy Physics - Phenomenology · Physics 2025-07-16 Atri Bhattacharya , Mary Hall Reno , Ina Sarcevic

Although the main features of the evolution of binary neutron star systems are now well established, many details are still subject to debate, especially regarding the post-merger phase. In particular, the lifetime of the hyper-massive…

High Energy Astrophysical Phenomena · Physics 2020-06-09 Matteo Lucca , Laura Sagunski

New calculations of the time evolution and isotopic composition for a network of nuclear reactions breathe new life into an old idea in nuclear fusion, burning solid room temperature lithium-6 deuteride ($^6$LiD) with neutrons. Modern-day…

Muon catalyzed fusion ($\mu$CF) has recently regained considerable research interest owing to several new developments and applications. In this regard, we have performed a comprehensive study of the most important fusion reaction, namely…

Nuclear Theory · Physics 2023-04-05 M. Kamimura , Y. Kino , T. Yamashita

If the gravitino is the lightest supersymmetric particle and the long-lived next-to-lightest sparticle (NSP) is the stau, the charged partner of the tau lepton, it may be metastable and form bound states with several nuclei. These bound…

Three light sterile neutrinos (\nu_e^s, \nu_\mu^s and \nu_\tau^s) are introduced to accommodate all the available neutrino data: the atmospheric neutrino anomaly is explained by \nu_\mu-\nu_\mu^s oscillation with maximal mixing; the solar…

High Energy Physics - Phenomenology · Physics 2009-11-07 Chun Liu , Jeonghyeon Song

When SUSY breaking produces only dimension-2 operators, gluino and photino masses are of order 1 GeV or less. The gluon-gluino bound state has mass 1.3-2.2 GeV and lifetime > 10^{-5} - 10^{-10} s. This range of mass and lifetime is largely…

High Energy Physics - Phenomenology · Physics 2008-11-26 Glennys R. Farrar