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Related papers: Gravity-mediated (or Composite) Dark Matter Confro…

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We point out that, in a class of gauge mediation models using metastable supersymmetry breaking vacua, the minimum of the supersymmetry breaking field in the early universe is dynamically deviated from the one in the low energy. The…

High Energy Physics - Phenomenology · Physics 2007-10-11 Motoi Endo , Fuminobu Takahashi

We propose an economical model to explain the apparent 130 GeV gamma ray peak, found in the Fermi/LAT data, in terms of dark matter annihilation through a dipole moment interaction. The annihilating dark matter particles represent a…

High Energy Physics - Phenomenology · Physics 2015-06-11 James M. Cline , Andrew R. Frey , Guy D. Moore

Dark matter annihilation into charged particles is necessarily accompanied by gamma rays, produced via radiative corrections. Internal bremsstrahlung from the final state particles can produce hard gamma rays up to the dark matter mass,…

Astrophysics · Physics 2010-02-01 Nicole F. Bell , Thomas D. Jacques

Several cosmic ray experiments have measured excesses in electrons and positrons, relative to standard backgrounds, for energies from ~ 10 GeV - 1 TeV. These excesses could be due to new astrophysical sources, but an explanation in which…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Spencer Chang , Lisa Goodenough

This paper investigates the parameter space of theories with gauge mediated supersymmetry breaking leading to gravitino (cold) dark matter with mass m_{3/2}= 1keV - 10MeV. We pay particular attention to the cosmological role of messenger…

High Energy Physics - Phenomenology · Physics 2009-11-11 Karsten Jedamzik , Martin Lemoine , Gilbert Moultaka

We infer dark matter properties from gamma ray residuals extracted using eight different interstellar emission scenarios proposed by the Fermi-LAT Collaboration to explain the Galactic Center gamma ray excess. Adopting the most plausible…

High Energy Physics - Phenomenology · Physics 2017-03-08 Csaba Balázs , Tong Li

We introduce a novel dark matter scenario where the visible sector and the dark sector share a common asymmetry. The two sectors are connected through an unstable mediator with baryon number one, allowing the standard model baryon asymmetry…

High Energy Physics - Phenomenology · Physics 2016-03-16 Nayara Fonseca , Lina Necib , Jesse Thaler

The existence of Dark Matter (DM) is a well established fact since many decades, thanks to the observation of the effects of its gravitational interaction with the ordinary matter in the Universe. However, our knowledge of the Dark Matter…

High Energy Physics - Phenomenology · Physics 2020-09-08 Alessandra Filippi , Marzio De Napoli

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

Astrophysics · Physics 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

We consider a simple class of models in which the dark matter, X, is coupled to a new gauge boson, phi, with a relatively low mass (m_phi \sim 100 MeV-3 GeV). Neither the dark matter nor the new gauge boson have tree-level couplings to the…

High Energy Physics - Phenomenology · Physics 2013-05-30 Dan Hooper , Neal Weiner , Wei Xue

We consider axion-mediated dark matter models motivated by Fermi gamma ray line at 130 GeV, where anomaly interactions of an axion-like scalar mediate a singlet Dirac fermion dark matter (DM) to electroweak gauge bosons. In these models,…

High Energy Physics - Phenomenology · Physics 2015-06-11 Hyun Min Lee , Myeonghun Park , Wan-Il Park

We review progress in understanding dark matter by astrophysics, and particularly via the effect of gravitational lensing. Evidence from many different directions now all imply that five sixths of the material content of the universe is in…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Richard Massey , Thomas Kitching , Johan Richard

We explore the feasibility and astrophysical consequences of a new long-range U(1) gauge field ("dark electromagnetism") that couples only to dark matter, not to the Standard Model. The dark matter consists of an equal number of positive…

High Energy Physics - Phenomenology · Physics 2009-11-13 Lotty Ackerman , Matthew R. Buckley , Sean M. Carroll , Marc Kamionkowski

In recent works, we have proposed a possible dark matter in composite messenger gauge mediation models. In this paper, we discuss the details of a composite messenger model taking a possible supersymmetry breaking scenario and show that the…

High Energy Physics - Phenomenology · Physics 2010-05-12 Koichi Hamaguchi , Eita Nakamura , Satoshi Shirai , Tsutomu T. Yanagida

We study for the first time the possibility that Dark Matter (represented by particles with spin $0,1/2$ or $1$) interacts gravitationally with Standard Model particles in an extra-dimensional Clockwork/Linear Dilaton model. We assume that…

High Energy Physics - Phenomenology · Physics 2020-04-13 Miguel G. Folgado , Andrea Donini , Nuria Rius

Gravitational positivity bounds provide consistency conditions for effective field theories with gravity. They turn out to be phenomenologically useful by providing lower bounds in parameters of new physics beyond the Standard Models (BSM).…

High Energy Physics - Phenomenology · Physics 2025-01-24 Suro Kim , Pyungwon Ko

In our current best cosmological model, the vast majority of matter in the Universe is dark, consisting of yet undetected, non-baryonic particles that do not interact electro-magnetically. So far, the only significant evidence for dark…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-09 Jenny Wagner

We address the question of gravitino dark matter in the context of gauge mediated supersymmetry breaking models.

High Energy Physics - Phenomenology · Physics 2007-12-21 G. Moultaka

The first published Fermi large area telescope (Fermi-LAT) measurement of the isotropic diffuse gamma-ray emission is in good agreement with a single power law, and is not showing any signature of a dominant contribution from dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 LAT collaboration , A. A. Abdo , M. Ackermann , M. Ajello , L. Baldini , J. Ballet , G. Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , B. Berenji , R. D. Blandford , E. D. Bloom , E. Bonamente , A. W. Borgland , A. Bouvier , J. Bregeon , A. Brez , M. Brigida , P. Bruel , T. H. Burnett , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , S. Carrigan , J. M. Casandjian , C. Cecchi , O. C. Elik , A. Chekhtman , C. C. Cheung , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , S. Cutini , C. D. Dermer , A. de Angelis , F. de Palma , S. W. Digel , E. do Couto e Silva , P. S. Drell , R. Dubois , D. Dumora , Y. Edmonds , C. Farnier , C. Favuzzi , S. J. Fegan , W. B. Focke , P. Fortin , M. Frailis , Y. Fukazawa , P. Fusco , F. Gargano , D. Gasparrini , N. Gehrels , S. Germani , N. Giglietto , F. Giordano , T. Glanzman , G. Godfrey , J. E. Grove , L. Guillemot , S. Guiriec , M. Gustafsson , D. Hadasch , A. K. Harding , D. Horan , R. E. Hughes , A. S. Johnson , W. N. Johnson , T. Kamae , H. Katagiri , J. Kataoka , N. Kawai , M. Kerr , J. Knodlseder , M. Kuss , J. Lande , L. Latronico , M. Llena Garde , F. Longo , F. Loparco , B. Lott , M. N. Lovellette , P. Lubrano , A. Makeev , M. N. Mazziotta , J. E. McEnery , C. Meurer , P. F. Michelson , W. Mitthumsiri , T. Mizuno , C. Monte , M. E. Monzani , A. Morselli , I. V. Moskalenko , S. Murgia , P. L. Nolan , J. P. Norris , E. Nuss , T. Ohsugi , N. Omodei , E. Orlando , J. F. Ormes , D. Paneque , J. H. Panetta , D. Parent , V. Pelassa , M. Pepe , M. Pesce-Rollins , F. Piron , S. Raino , R. Rando , A. Reimer , O. Reimer , T. Reposeur , A. Y. Rodriguez , M. Roth , H. F. W. Sadrozinski , A. Sander , P. M. Saz Parkinson , J. D. Scargle , A. Sellerholm , C. Sgro , E. J. Siskind , P. D. Smith , G. Spandre , P. Spinelli , J. L. Starck , M. S. Strickman , D. J. Suson , H. Takahashi , T. Tanaka , J. B. Thayer , J. G. Thayer , D. F. Torres , Y. Uchiyama , T. L. Usher , V. Vasileiou , N. Vilchez , V. Vitale , A. P. Waite , P. Wang , B. L. Winer , K. S. Wood , T. Ylinen , G. Zaharijas , M. Ziegle

Dark matter annihilation into photons in our galaxy would constitute an exciting indirect signal of its existence, as underscored by tentative evidence for 130 GeV dark matter in Fermi/LAT data. Models that give a large annihilation cross…

High Energy Physics - Phenomenology · Physics 2013-11-11 James M. Cline , Grace Dupuis , Zuowei Liu