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Related papers: Astrophysical limits on light NMSSM neutralinos

200 papers

We study the neutralino sector of the Minimal Non-minimal Supersymmetric Standard Model (MNSSM) where the $\mu$ problem of the Minimal Supersymmetric Standard Model (MSSM) is solved without accompanying problems related with the appearance…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Hesselbach , D. J. Miller , G. Moortgat-Pick , R. Nevzorov , M. Trusov

We discuss the prospects for detecting supersymmetric particles in variants of the minimal supersymmetric extension of the Standard Model (MSSM), in light of laboratory and cosmological constraints. We first assume that the lightest…

High Energy Physics - Phenomenology · Physics 2009-09-11 John Ellis , Keith A. Olive , Yudi Santoso , Vassilis C. Spanos

We study the phenomenology of neutralino dark matter within generic supersymmetric scenarios where the Gaugino and Higgsino masses are much lighter than the scalar soft breaking masses (Split Supersymmetry). We consider a low-energy…

High Energy Physics - Phenomenology · Physics 2007-05-23 Antonio Masiero , Stefano Profumo , Piero Ullio

Dark matter is a key piece of the current cosmological scenario, with weakly interacting massive particles (WIMPs) a leading dark matter candidate. WIMPs have not been detected in their conventional parameter space (100 GeV $\lesssim…

We consider the possibility that the cosmological dark matter consists of particles very close in mass to new colored particles below the TeV scale. While such a scenario is inherently difficult to directly confirm at colliders, we find…

High Energy Physics - Phenomenology · Physics 2012-03-05 Masaki Asano , Torsten Bringmann , Christoph Weniger

We present statistically convergent profile likelihood maps obtained via global fits of a phenomenological Minimal Supersymmetric Standard Model with 15 free parameters (the MSSM-15), based on over 250M points. We derive constraints on the…

High Energy Physics - Phenomenology · Physics 2015-06-19 C. Strege , G. Bertone , G. J. Besjes , S. Caron , R. Ruiz de Austri , A. Strubig , R. Trotta

Recent results from direct and indirect searches for dark matter (DM) have motivated the study of particle physics models that can provide weakly interacting massive particles (WIMPs) in the mass range 1-50 GeV. Viable candidates for light…

High Energy Physics - Phenomenology · Physics 2014-08-05 D. G. Cerdeno , M. Peiro , S. Robles

Uncertainties of the MSSM predictions are due to an unknown SUSY breaking mechanism. To reduce these uncertainties, one usually imposes constraints on the MSSM parameter space. Recently, two new constraints became available, both from…

High Energy Physics - Phenomenology · Physics 2009-11-11 D. Yu. Bogachev , A. V. Gladyshev , D. I. Kazakov , A. S. Nechaev

Cosmic-ray observations provide a powerful probe of dark matter annihilation in the Galaxy. In this paper we derive constraints on heavy dark matter from the recent precise AMS-02 antiproton data. We consider all possible annihilation…

High Energy Physics - Phenomenology · Physics 2018-04-23 Alessandro Cuoco , Jan Heisig , Michael Korsmeier , Michael Krämer

The prediction of neutralino dark matter is generally regarded as one of the successes of the Minimal Supersymmetric Standard Model (MSSM). However the successful regions of parameter space allowed by WMAP and collider constraints are quite…

High Energy Physics - Phenomenology · Physics 2009-11-11 S. F. King , J. P. Roberts

We study the constraints on neutralino dark matter in minimal low energy supersymmetry models and the case of heavy lepton and quark scalar superpartners. For values of the Higgsino and gaugino mass parameters of the order of the weak…

High Energy Physics - Phenomenology · Physics 2017-05-31 Peisi Huang , Roger A. Roglans , Daniel D. Spiegel , Yitian Sun , Carlos E. M. Wagner

We examine indirect signals produced by neutralino self-annihilations, in the galactic halo or inside celestial bodies, in the frame of an effective MSSM model without gaugino-mass unification at a grand unification scale. We compare our…

High Energy Physics - Phenomenology · Physics 2009-11-10 A. Bottino , F. Donato , N. Fornengo , S. Scopel

After a short introduction on particle candidates for dark matter within possible extensions of the standard model, we concentrate on Weakly Interacting Massive Particles, and on one of their most interesting physical realizations: the…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Bottino , F. Donato , N. Fornengo , S. Scopel

The content of matter in the Universe is estimated to be the 27% of its critical density. It is almost universally accepted that most ot this matter is non-baryonic. Constraints from primordial nucleosynthesis and cosmic background…

Astrophysics · Physics 2015-06-24 E. Bisesi , M. Mariotti , V. Scalzotto

The negative outcome of searches for supersymmetry performed at LEP have been used to derive indirect constraints on the parameters of the most plausible supersymmetric candidates for cold dark matter, in particular for the lightest…

High Energy Physics - Experiment · Physics 2007-05-23 Gerardo Ganis

We highlight the differences of the dark matter sector between the constrained minimal supersymmetric SM (CMSSM) and the next-to-minimal supersymmetric SM (NMSSM) including the 126 GeV Higgs boson using GUT scale parameters. In the dark…

High Energy Physics - Phenomenology · Physics 2015-12-30 C. Beskidt , W. de Boer , D. I. Kazakov

We report on the observations of 14 dwarf spheroidal galaxies with the Fermi Gamma-Ray Space Telescope taken during the first 11 months of survey mode operations. The Fermi telescope provides a new opportunity to test particle dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-17 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 , J. Bregeon , A. Brez , M. Brigida , P. Bruel , T. H. Burnett , S. Buson , G. A. Caliandro , R. A. Cameron , P. A. Caraveo , J. M. Casandjian , C. Cecchi , A. Chekhtman , C. C. Cheung , J. Chiang , S. Ciprini , R. Claus , J. Cohen-Tanugi , J. Conrad , A. de Angelis , F. de Palma , S. W. Digel , E. do Couto e Silva , P. S. Drell , A. Drlica-Wagner , R. Dubois , D. Dumora , C. Farnier , C. Favuzzi , S. J. Fegan , W. B. Focke , P. Fortin , M. Frailis , Y. Fukazawa , P. Fusco , F. Gargano , N. Gehrels , S. Germani , B. Giebels , N. Giglietto , F. Giordano , T. Glanzman , G. Godfrey , I. A. Grenier , J. E. Grove , L. Guillemot , S. Guiriec , M. Gustafsson , A. K. Harding , E. Hays , D. Horan , R. E. Hughes , M. S. Jackson , T. E. Jeltema , G. Johannesson , A. S. Johnson , R. P. Johnson , W. N. Johnson , T. Kamae , H. Katagiri , J. Kataoka , M. Kerr , J. Knodlseder , M. Kuss , J. Lande , L. Latronico , M. Lemoine-Goumard , F. Longo , F. Loparco , B. Lott , M. N. Lovellette , P. Lubrano , G. M. Madejski , 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 , E. Moretti , 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 , T. A. Porter , S. Profumo , S. Raino , R. Rando , M. Razzano , A. Reimer , O. Reimer , T. Reposeur , 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. Sgro , E. J. Siskind , D. A. Smith , P. D. Smith , G. Spandre , P. Spinelli , M. S. Strickman , D. J. Suson , H. Takahashi , T. Takahashi , T. Tanaka , J. B. Thayer , J. G. Thayer , D. J. Thompson , L. Tibaldo , D. F. Torres , A. Tramacere , 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 , James S. Bullock , Manoj Kaplinghat , Gregory D. Martinez

The neutralino sector of the semi-constrained next-to-minimal supersymmetric standard model is explored under recent experimental constraints, with special attention to dark matter (DM) limits. The effects of the upper and lower bounds of…

High Energy Physics - Phenomenology · Physics 2021-02-02 Elham Aldufeery , Maien Binjonaid

Current data (LHC direct searches, Higgs mass, dark matter-related bounds) severely affect the constrained minimal SUSY standard model (CMSSM) with neutralinos as dark matter candidates. But the evidence for neutrino masses coming from…

High Energy Physics - Phenomenology · Physics 2016-07-22 Shankha Banerjee , Geneviève Bélanger , Biswarup Mukhopadhyaya , Pasquale D. Serpico

While most BSM searches at the LHC focus on heavy new states, the NMSSM contains the possibility of new light states that have escaped detection due to their singlet nature. Here we focus on light pseudoscalars, investigating the parameter…

High Energy Physics - Phenomenology · Physics 2017-09-11 Robin Aggleton , Daniele Barducci , Nils-Erik Bomark , Stefano Moretti , Claire Shepherd-Themistocleous