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Related papers: Ultra-high energy LSP

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We suggest that supersymmetric dark matter be used to set the energy scale of a linear $e^+ e^-$ collider. Assuming that the lightest supersymmetric particle (LSP) is a stable neutralino $\chi$, as in many incarnations of the MSSM with…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , Gerardo Ganis , Keith A. Olive

We discuss the production of ultra high energy neutrinos coming from the propagation of ultra high energy cosmic rays and in the framework of top-down models for the production of these extremely energetic particles. We show the importance…

High Energy Astrophysical Phenomena · Physics 2016-03-21 Roberto Aloisio

We summarize the current status and future prospects for low energy (weak scale) supersymmetry. In particular, we evaluate the capabilities of various $e^+e^-$, $p\bar p$ and $pp$ colliders to discover evidence for supersymmetric particles.…

Searches for pair production of squarks, sleptons, charginos, and neutralinos are performed with the data collected by the ALEPH detector at LEP at centre-of-mass energies from 188.6 to 201.6 GeV. No evidence for any such signals is…

High Energy Physics - Experiment · Physics 2012-08-27 ALEPH Collaboration

One way to suppress flavor changing neutral currents or CP violating processes in supersymmetry is to make at least some of the first two generations' scalars superheavy (above ~20 TeV). We summarize the motivations and challenges,…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sandro Ambrosanio , James D. Wells

In this thesis, I describe in great detail the physics of the decay of any Super-Heavy X particle (with masses up to the grand unification scale ~ 10^16 GeV and possibly beyond), and the computer code I developed to model this process -…

High Energy Physics - Phenomenology · Physics 2007-05-23 Cyrille Barbot

We study supersymmetric scenarios where the dark matter is the gaugino of an unbroken hidden U(1) which interacts with the visible world only via a small kinetic mixing with the hypercharge. Strong constraints on the parameter space can be…

High Energy Physics - Phenomenology · Physics 2009-02-12 A. Ibarra , A. Ringwald , C. Weniger

It is proposed that the highest energy $\sim 10^{20}$eV cosmic ray primaries are protons, decay products of a long-lived progenitor whose high kinetic energy arises from decay of a distant (cosmological) superheavy particle, G. Such a…

Astrophysics · Physics 2007-05-23 Paul H. Frampton

Searches for supersymmetric particles at LEP are first reviewed, with some emphasis on the mass limit for the lightest neutralino. The framework is the MSSM with R-parity conservation, with brief excursions towards mSUGRA and GMSB. Next,…

High Energy Physics - Experiment · Physics 2007-05-23 J. -F. Grivaz

We study supersymmetric extensions of the Standard Model with small R-parity and lepton number violating couplings which are naturally consistent with primordial nucleosynthesis, thermal leptogenesis and gravitino dark matter. We consider…

High Energy Physics - Phenomenology · Physics 2011-11-30 S. Bobrovskyi , W. Buchmuller , J. Hajer , J. Schmidt

We investigate the cosmological gravitino problem in gauge-mediated supersymmetry breaking models, where the gravitino becomes in general the lightest supersymmetric particle (LSP). In order to avoid the overclosure of the stable gravitino,…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Asaka , K. Hamaguchi , Koshiro Suzuki

We propose an explanation for the recently reported ultra-high-energy neutrino signal at KM3NeT, which shows no clear association with known astrophysical sources. While decaying dark matter in the Galactic Center is a natural candidate,…

High Energy Physics - Phenomenology · Physics 2026-02-02 Yongsoo Jho , Seong Chan Park , Chang Sub Shin

We investigate the idea that ultrahigh energy gamma-rays (E>10 TeV) can be produced when charged particles are accelerated by microscopic black holes. We begin by showing that microscopic black holes may exist as remnants of primordial…

Astrophysics · Physics 2009-11-07 Roberto Casadio , Benjamin Harms , Octavian Micu

The highest energy cosmic rays observed possess macroscopic energies and their origin is likely to be associated with the most energetic processes in the Universe. Their existence triggered a flurry of theoretical explanations ranging from…

High Energy Physics - Phenomenology · Physics 2014-11-17 Guenter Sigl

The sources and fluxes of superGZK neutrinos, $E>10^{20}$ eV, are discussed. The fluxes of {\em cosmogenic neutrinos}, i.e. those produced by ultra-high energy cosmic rays (UHECR) interacting with CMB photons, are calculated in the models,…

Astrophysics · Physics 2007-05-23 V. Berezinsky

An intriguing possibility for TeV scale physics is the existence of neutral long lived particles (LOLIPs) that subsequently decay into SM states. Such particles are many cases indistinguishable from missing transverse energy (MET) at…

High Energy Physics - Phenomenology · Physics 2014-11-20 Patrick Meade , Shmuel Nussinov , Michele Papucci , Tomer Volansky

The origin of Ultra--High Energy ($E \gsim 10^{20}$ eV) Cosmic Rays (UHECR) remains mysterious. I discuss ``top--down'' models, where UHECR originate from the decay of very massive, long--lived particles. I summarize the calculation of the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Manuel Drees

The results of a search for top squark (stop) pair production in final states with one isolated lepton, jets, and missing transverse momentum are reported. The analysis is performed with proton--proton collision data at $\sqrt{s} = 8$ TeV…

High Energy Physics - Experiment · Physics 2014-12-05 ATLAS Collaboration

The presence of a Higgsino-like neutralino next-to-lightest sparticle (NLSP) and a keV scale gravitino ($\widetilde{G}$) LSP opens up new decay modes of the NLSP, mainly to a Higgs/$Z$ boson and the LSP. Besides, a keV-scale gravitino as a…

High Energy Physics - Phenomenology · Physics 2020-04-29 Juhi Dutta , Biswarup Mukhopadhyaya , Santosh Kumar Rai

If dark matter neutral LSPs in the galactic halo decay into two body final states containing photons or neutrinos they could be detected even if the decay rates are very small, 10**{-32} per sec. I calculate mass and lifetime bounds from…

Astrophysics · Physics 2011-04-15 M. V. Diwan
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