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Related papers: Gamma Ray Constraints on Flavor Violating Asymmetr…

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For the first time, the Fermi-LAT measured the angular power spectrum (APS) of anisotropies in the diffuse gamma-ray background. The data is found to be broadly compatible with a model with contributions from the point sources in the 1-year…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Mattia Fornasa , Jesus Zavala , Miguel A. Sanchez-Conde , Francisco Prada , Mark Vogelsberger

The cosmic-ray excess observed by PAMELA in the positron fraction and by FERMI and HESS in the electron + positron flux can be interpreted in terms of DM annihilations or decays into leptonic final states. Final states into tau's or 4mu…

High Energy Physics - Phenomenology · Physics 2010-02-24 Patrick Meade , Michele Papucci , Alessandro Strumia , Tomer Volansky

Measuring high energy cosmic ray electrons/positrons (CRE) provides important means for the dark matter (DM) indirect detection and for probing the nearby galactic sources. In this work, we perform a systematic analysis of the flavor…

High Energy Astrophysical Phenomena · Physics 2020-08-25 Shao-Feng Ge , Hong-Jian He , Yu-Chen Wang , Qiang Yuan

The detailed origin of the diffuse gamma-ray background is still unknown. However, the contribution of unresolved sources is expected to induce small-scale anisotropies in this emission, which may provide a way to identify and constrain the…

High Energy Astrophysical Phenomena · Physics 2019-08-15 G. A. Gomez-Vargas , A. Cuoco , T. Linden , M. A. Sanchez-Conde , J. M. Siegal-Gaskins , T. Delahaye , M. Fornasa , E. Komatsu , F. Prada , J. Zavala

We propose an unified model of dark matter and baryon asymmetry in a lepto-philic world above the electroweak scale. We provide an example where the inflaton decay products subsequently generate a lepton asymmetry and a dark matter…

High Energy Physics - Phenomenology · Physics 2009-11-06 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu , Philip Stephens

The decay of dark matter is predicted by many theoretical models and can produce observable contributions to the cosmic-ray fluxes. I shortly discuss the interpretation of the positron and electron excess as observed by PAMELA and Fermi LAT…

High Energy Physics - Phenomenology · Physics 2009-10-30 Christoph Weniger

Recently, a preliminary spectrum from the Fermi Gamma-ray Space Telescope has been presented for the inner galaxy (-30 < l < 30, -5 < b < 5), as well as the galactic center (-1 < l < 1, -1< b < 1). We consider the implications of these data…

High Energy Astrophysical Phenomena · Physics 2009-07-29 Ilias Cholis , Gregory Dobler , Douglas P. Finkbeiner , Lisa Goodenough , Tracy R. Slatyer , Neal Weiner

In supersymmetric theories without R-parity, the gravitino can play the role of a decaying Dark Matter candidate without the problem of late NLSP decays affecting Big Bang Nucleosynthesis. In this work, we elaborate on recently discussed…

High Energy Physics - Phenomenology · Physics 2014-08-26 Angelo Monteux , Eric Carlson , Jonathan Cornell

The observation of cosmic sub-PeV gamma-rays from the Crab Nebula opens up the possibility of testing cosmic ray photon transparency at the multi-hundred TeV scale. Assuming no deviation from a source gamma-ray emission due to accelerated…

High Energy Astrophysical Phenomena · Physics 2021-03-03 Xiao-Jun Bi , Yu Gao , Junguang Guo , Nick Houston , Tianjun Li , Fangzhou Xu , Xin Zhang

The lepton and dilepton charge asymmetries from $B_{d}$ and $B_{s}$ are predicted to be small in the standard model, whereas new physics could increase their values significantly. In this paper, we explore the use of the lepton asymmetries…

High Energy Physics - Phenomenology · Physics 2009-09-15 Lisa Randall , Shufang Su

Recent results from the PAMELA experiment indicate an excess in the positron spectrum above 10 GeV, but anti-proton data are consistent with the expected astrophysical backgrounds. We propose a scenario that reproduces these features. Dark…

High Energy Physics - Phenomenology · Physics 2009-09-24 Daniel J. Phalen , Aaron Pierce , Neal Weiner

We discuss the cosmic ray spectra in annihilating/decaying Nambu-Goldstone dark matter models. The recent observed positron/electron excesses at PAMELA and Fermi experiments are well fitted by the dark matter with a mass of 3TeV for the…

High Energy Physics - Phenomenology · Physics 2009-12-04 Masahiro Ibe , Hitoshi Murayama , Satoshi Shirai , Tsutomu T. Yanagida

Several classes of astrophysical sources contribute to the approximately isotropic gamma-ray background measured by the Fermi Gamma-Ray Space Telescope. In this paper, we use Fermi's catalog of gamma-ray sources (along with corresponding…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 Ilias Cholis , Dan Hooper , Samuel D. McDermott

Gamma rays reveal extreme, nonthermal conditions in the Universe. The Fermi Gamma-ray Space Telescope has been exploring the gamma-ray sky for more than four years, enabling a search for powerful transients like gamma-ray bursts, solar…

High Energy Astrophysical Phenomena · Physics 2015-06-16 D. J. Thompson

Gamma-rays from cosmological sources contain information about gamma-ray interactions. Standard model and non-standard model photon interactions along the path between the source and the observer can lead to changes in the energy or state…

High Energy Astrophysical Phenomena · Physics 2014-08-19 Rebecca Reesman , T. P. Walker

Dark matter (DM) particle annihilation or decay can produce monochromatic $\gamma$-rays readily distinguishable from astrophysical sources. $\gamma$-ray line limits from 30 GeV to 200 GeV obtained from 11 months of Fermi Large Area Space…

High Energy Astrophysical Phenomena · Physics 2012-05-15 The Fermi LAT Collaboration , A. A. Abdo , M. Ackermann , M. Ajello , W. B. Atwood , L. Baldini , J. Ballet , G. Barbiellini , D. Bastieri , K. Bechtol , R. Bellazzini , B. Berenji , 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 , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , C. D. Dermer , A. de Angelis , F. de Palma , S. W. Digel , E. do Couto e Silva , P. S. Drell , A. Drlica-Wagner , R. Dubois , D. Dumora , Y. Edmonds , R. Essig , C. Farnier , C. Favuzzi , S. J. Fegan , W. B. Focke , P. Fortin , M. Frailis , Y. Fukazawa , S. Funk , P. Fusco , F. Gargano , D. Gasparrini , N. Gehrels , S. Germani , N. Giglietto , F. Giordano , T. Glanzman , G. Godfrey , I. A. Grenier , J. E. Grove , L. Guillemot , S. Guiriec , M. Gustafsson , D. Hadasch , A. K. Harding , D. Horan , R. E. Hughes , M. S. Jackson , G. J . ohannesson , A. S. Johnson , R. P. Johnson , W. N. Johnson , T. Kamae , H. Katagiri , J. Kataoka , N. Kawai , M. Kerr , J. Kno . dlseder , 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 , A. A. Moiseev , 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 , M. Ozaki , D. Paneque , J. H. Panetta , D. Parent , V. Pelassa , M. Pepe , M. Pesce-Rollins , F. Piron , S. Rainó , R. Rando , M. Razzano , A. Reimer , O. Reimer , T. Reposeur , J. Ripken , S. Ritz , A. Y. Rodriguez , M. Roth , H. F. -W. Sadrozinski , A. Sander , P. M. Saz Parkinson , J. D. Scargle , T. L. Schalk , A. Sellerholm , C. Sgró , E. J. Siskind , D. A. Smith , P. D. Smith , G. Spandre , P. Spinelli , J. -L. Starck , M. S. Strickman , D. J. Suson , H. Tajima , H. Takahashi , T. Tanaka , J. B. Thayer , J. G. Thayer , L. Tibaldo , 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 , M. Ziegler

Dark matter annihilation is one of the leading explanations for the recently observed $e^\pm$ excesses in cosmic rays by PAMELA, ATIC, FERMI-LAT and HESS. Any dark matter annihilation model proposed to explain these data must also explain…

High Energy Physics - Phenomenology · Physics 2010-04-29 Xiao-Jun Bi , Xiao-Gang He , Ernest Ma , Juan Zhang

We discuss charged lepton flavour violating processes such as mu -> e gamma in supersymmetric extensions of the Standard Model and in models with gauge-Higgs unification and a warped extra dimension. In both classes of models the processes…

High Energy Physics - Phenomenology · Physics 2015-06-17 C. Hagedorn

The anomalies observed in recent cosmic ray experiments seem to strongly constrain the nature of the dark matter. In this letter, we investigate a possibility of the fermionic dark matter with a minimal extension of the standard model. We…

High Energy Physics - Phenomenology · Physics 2010-04-30 Koichi Hamaguchi , Satoshi Shirai , T. T. Yanagida

Guided by gauge principles we discuss a predictive and falsifiable UV complete model where the Dirac fermion that accounts for the cold dark matter abundance in our universe induces the lepton flavor violation (LFV) decays $\mu \rightarrow…

High Energy Physics - Phenomenology · Physics 2018-04-25 Giorgio Arcadi , C. P. Ferreira , Florian Goertz , M. M. Guzzo , Farinaldo S. Queiroz , A. C. O. Santos
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