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The CiADS-BDE is a beam-dump experiment recently proposed for searching for light, long-lived particles (LLPs) at China initiative Accelerator Driven System. Primarily thanks to the large numbers of protons on target at the experiment, it…

High Energy Physics - Phenomenology · Physics 2025-01-28 Zeren Simon Wang , Yu Zhang , Liangwen Chen

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

High Energy Physics - Phenomenology · Physics 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

Two leading dark matter candidates from supersymmetry and other theories of physics beyond the standard model are WIMPs and weak scale gravitinos. If the lightest stable particle is a gravitino, then a WIMP will decay into it with a natural…

Astrophysics · Physics 2008-11-26 Manoj Kaplinghat

Unstable heavy particles well above the TeV scale are unaccessible experimentally. So far, Big-Bang Nucleosynthesis (BBN) provides the strongest limits on their mass and lifetime, the latter being shorter than 0.1 second. We show how these…

High Energy Physics - Phenomenology · Physics 2020-07-22 Yann Gouttenoire , Géraldine Servant , Peera Simakachorn

Dark matter scenarios are being tested at the LHC in the general-purpose experiments through promptly decaying states. In parallel, new dedicated detectors have been proposed for the LHC to probe dark matter portal theories predicting…

High Energy Physics - Experiment · Physics 2023-01-27 Vasiliki A. Mitsou

In the present work we examine the implications on dark matter searches of the possibility of a partial decay of a neutron into a dark matter particle, slightly lighter than itself. Such a scenario recently proposed is required to bridge…

High Energy Physics - Phenomenology · Physics 2020-05-15 J. D. Vergados

We review important reactions in the big bang nucleosynthesis (BBN) model involving a long-lived negatively charged massive particle, $X^-$, which is much heavier than nucleons. This model can explain the observed $^7$Li abundances of…

Cosmology and Nongalactic Astrophysics · Physics 2017-09-20 Motohiko Kusakabe , Grant. J. Mathews , Toshitaka Kajino , Myung-Ki Cheoun

The collision of a high energy cosmic ray with a nucleon in the upper atmosphere could produce long-lived heavy particles. Such particles would be very penetrating, since the energy loss in matter scales as the inverse mass, and could reach…

High Energy Physics - Phenomenology · Physics 2008-11-26 Markus Ahlers , Jose Ignacio Illana , Manuel Masip , Davide Meloni

We investigate new and unusual signals that arise in theories where dark matter is asymmetric and carries a net antibaryon number, as may occur when the dark matter abundance is linked to the baryon abundance. Antibaryonic dark matter can…

High Energy Physics - Phenomenology · Physics 2014-01-14 Hooman Davoudiasl , David E. Morrissey , Kris Sigurdson , Sean Tulin

Recent models invoking extra spacelike dimensions inhabited by (bulk) neutrinos are shown to have significant cosmological effects if the size of the largest extra dimension is R > 1 fm. We consider effects on cosmic microwave background…

High Energy Physics - Phenomenology · Physics 2009-10-31 Kevork Abazajian , George M. Fuller , Mitesh Patel

An analysis of radiative decays of the neutrinos $\nu_j\to \nu_l \gamma$ is discussed in MSSM extensions with a vector like lepton generation. Specifically we compute neutrino decays arising from the exchange of charginos and charged…

High Energy Physics - Phenomenology · Physics 2013-08-09 Amin Aboubrahim , Tarek Ibrahim , Pran Nath

The Big Bang nucleosynthesis (BBN) in the presence of charged massive particles (CHAMPs) is studied in detail. All currently known effects due to the existence of bound states between CHAMPs and nuclei, including possible late-time…

High Energy Physics - Phenomenology · Physics 2009-06-19 Karsten Jedamzik

We calculate the early universe evolution of perturbations in the dark matter energy density in the context of simple dark sector models containing a GeV scale light mediator. We consider the case that the mediator is long lived, with…

High Energy Physics - Phenomenology · Physics 2015-05-08 Yue Zhang

Future cosmological data may be sensitive to the effects of a finite sum of neutrino masses even as small as ~0.06 eV, the lower limit guaranteed by neutrino oscillation experiments. We show that a cosmological detection of neutrino mass at…

Astrophysics · Physics 2008-11-26 Pasquale D. Serpico

Any light relic which was in thermal equilibrium with the Standard Model before it freezes out results in a shift in the effective number of neutrino species, $N_{eff}$. This quantity is being measured with increasing precision, and planned…

High Energy Physics - Phenomenology · Physics 2023-09-14 Katarina Bleau , Joseph Bramante , Christopher Cappiello

The high-energy Universe is potentially a great laboratory for searching new light bosons such as axion-like particles (ALPs). Cosmic sources are indeed the scene of violent phenomena that involve strong magnetic field and/or very long…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Pierre Brun

We discuss a cosmology in which cold dark matter begins to decay into relativistic particles at a recent epoch (z < 1). We show that the large entropy production and associated bulk viscosity from such decays leads to an accelerating…

Astrophysics · Physics 2008-11-26 G. J. Mathews , N. Q. Lan , C. Kolda

Long-lived colored particles with masses m > 200 GeV are allowed by current accelerator searches, and are predicted by a number of scenarios for physics beyond the standard model. We argue that such "heavy partons'' effectively have a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Junhai Kang , Markus A. Luty , Salah Nasri

The radiative component of the Universe has a characteristic impact on both large scale structure (LSS) and the cosmic microwave background radiation (CMB). We use the recent WMAP data, together with previous CBI data and 2dF matter power…

Astrophysics · Physics 2009-11-07 Elena Pierpaoli

We show that a Majorana heavy neutrino with a mass O(100TeV) is a good candidate particle for cold dark matter. It can be responsible for the majority of the cosmological diffuse photon background owing to lifetime of the order of…

High Energy Physics - Phenomenology · Physics 2007-05-23 D. Palle
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