CERN Accelerating science

CERN Document Server 12 záznamov nájdených  1 - 10ďalší  skoč na záznam: Hľadanie trvalo 1.34 sekúnd. 
1.
Chapter 5 Dark Matter and New Physics Beyond the Standard Model with LHAASO / Bi, Xiao-Jun (Beijing, Inst. High Energy Phys.) ; Addazi, Andrea (SCU, Chengdu ; Frascati) ; Belotsky, Konstantin (Moscow Phys. Eng. Inst.) ; Beylin, Vitaly (Southern Federal U.) ; Cirelli, Marco (Paris, LPTHE) ; Esmaili, Arman (Rio de Janeiro, Pont. U. Catol.) ; Fornengo, Nicolao (INFN, Turin) ; Gan, Qing-Yu (SCU, Chengdu) ; Kachekriess, Michael (Norwegian U. Sci. Tech.) ; Khlopov, Maxim (APC, Paris ; Moscow Phys. Eng. Inst. ; Southern Federal U.) et al.
Abstract In order to reveal the nature of dark matter, it is crucial to detect its non-gravitational interactions with the standard model particles. The traditional dark matter searches focused on the so-called weakly interacting massive particles. [...]
2022 - 13 p. - Published in : Chin. Phys. C 46 (2022) 030005 Fulltext: PDF;
2.
Dark Matter Searches for heavy Dark Matter with LHAASO / Addazi, Andrea (Sichuan U. ; INFN, Rome) ; Belotsky, Konstantin (Moscow Phys. Eng. Inst.) ; Beylin, Vitaly (Southern Federal U.) ; Cirelli, Marco (Paris, LPTHE) ; DiSciascio, Giuseppe (INFN, Rome) ; Esmaili, Arman (Rio de Janeiro, Pont. U. Catol.) ; Fornengo, Nicolao (Turin U. ; INFN, Turin) ; Gan, Qingyu (Sichuan U.) ; Kachekriess, Michael (Norwegian U. Sci. Tech.) ; Khlopov, Maxim (APC, Paris ; Moscow Phys. Eng. Inst. ; Southern Federal U.) et al.
We discuss the implications of next future LHAASO data on searches of Heavy Dark Matter decays..
SISSA, 2021 - 8 p. - Published in : PoS ICRC2021 (2021) 574 Fulltext: PDF;
In : 37th International Cosmic Ray Conference (ICRC 2021), Berlin, Germany, 15 - 22 Jul 2021, pp.574
3.
Strongest model-independent bound on the lifetime of Dark Matter / Audren, Benjamin (ITPP, Lausanne) ; Lesgourgues, Julien (ITPP, Lausanne ; CERN ; Annecy, LAPTH) ; Mangano, Gianpiero (INFN, Naples) ; Serpico, Pasquale Dario (Annecy, LAPTH) ; Tram, Thomas (ITPP, Lausanne)
Dark Matter is essential for structure formation in the late Universe so it must be stable on cosmological time scales. But how stable exactly? Only assuming decays into relativistic particles, we report an otherwise model independent bound on the lifetime of Dark Matter using current cosmological data. [...]
arXiv:1407.2418; CERN-PH-TH-2014-105.- 2014 - 15 p. - Published in : JCAP 12 (2014) 028 Fulltext: PDF; External link: Preprint
4.
Gamma rays from Dark Matter Annihilation in the Central Region of the Galaxy / Serpico, Pasquale Dario (CERN) ; Hooper, Dan (Fermilab ; Chicago U., Astron. Astrophys. Ctr.)
In this article, we review the prospects for the Fermi satellite (formerly known as GLAST) to detect gamma rays from dark matter annihilations in the Central Region of the Milky Way, in particular on the light of the recent astrophysical observations and discoveries of Imaging Atmospheric Cherenkov Telescopes. While the existence of significant backgrounds in this part of the sky limits Fermi's discovery potential to some degree, this can be mitigated by exploiting the peculiar energy spectrum and angular distribution of the dark matter annihilation signal relative to those of astrophysical backgrounds..
arXiv:0902.2539; CERN-PH-TH-2009-025; FERMILAB-PUB-09-045-A; CERN-PH-TH-2009-025; FERMILAB-PUB-09-045-A.- Geneva : CERN, 2009 - 18 p. - Published in : New J. Phys.
Fulltext: njp9_10_105010 - PDF; arXiv:0902.2539 - PDF; External link: Fermilab Library Server (fulltext available)
5.
Possible causes of a rise with energy of the cosmic ray positron fraction / Serpico, Pasquale Dario (CERN)
Based on general considerations rather than model-dependent fits to specific scenarios, we argue that an increase with energy of the positron fraction in cosmic rays, suggested by several experiments at E>~10 GeV, most likely requires a primary source of electron-positron pairs. We discuss the possible alternatives, and find none of them plausible on astrophysical or particle physics grounds. [...]
arXiv:0810.4846; CERN-PH-TH-2009-007.- 2009 - 4 p. - Published in : Phys. Rev. D 79 (2009) 021302 APS Published version, local copy: PDF; Fulltext: PDF; External link: Preprint
6.
Pulsars as the Sources of High Energy Cosmic Ray Positrons / Hooper, Dan (Chicago U., Astron. Astrophys. Ctr. ; Fermilab) ; Blasi, Pasquale (Arcetri Observ. ; Fermilab ; Gran Sasso) ; Serpico, Pasquale Dario (CERN ; Fermilab)
Recent preliminary results from the PAMELA satellite indicate the presence of a large flux of positrons (relative to electrons) in the cosmic ray spectrum between approximately 10 and 50 GeV. As annihilating dark matter particles in many models are predicted to contribute to the cosmic ray positron spectrum in this energy range, a great deal of interest has resulted from this observation. [...]
arXiv:0810.1527; FERMILAB-PUB-08-429-A; CERN-PH-TH-2008-228; FERMILAB-PUB-08-429-A.- 2009 - 10 p. - Published in : JCAP 01 (2009) 025 Fulltext: PDF; IOP Open Access article: PDF; External link: Fermilab Library Server (fulltext available)
7.
A global autocorrelation study after the first Auger data : impact on the number density of UHECR sources / Cuoco, A (Aarhus U.) ; Hannestad, S (Aarhus U.) ; Haugboelle, T (Aarhus U.) ; Kachelriess, M (Fermilab) ; Serpico, Pasquale Dario (Fermilab ; CERN)
We perform an autocorrelation study of the Auger data with the aim to constrain the number density ns of ultrahigh energy cosmic ray (UHECR) sources, estimating at the same time the effect on ns of the systematic energy scale uncertainty and of the distribution of UHECR. The use of global analysis has the advantage that no biases are introduced, either in ns or in the related error bar, by the a priori choice of a single angular scale. [...]
arXiv:0809.4003; FERMILAB-PUB-08-315-A; IFT-UAM-CSIC-08-55; CERN-PH-TH-2009-106.- 2009 - 7 p. - Published in : Astrophys. J. 702 (2009) 825-832 External link: Preprint
8.
Synthesis of CNO elements in standard BBN / Iocco, F ; Serpico, Pasquale Dario
2006 - Published in : PoS: NIC-IX (2006) , pp. 201 Published version from PoS: PDF;
In : 9th International Symposium on Nuclear Astrophysic: Nuclei in the Cosmos, CERN, Geneva, Switzerland, 25 - 30 Jun 2006, pp.201
9.
Results on axion physics from the CAST Experiment at CERN / CAST Collaboration
Axions are expected to be produced in the sun via the Primakoff process. They may be detected through the inverse process in the laboratory, under the influence of a strong magnetic field, giving rise to X-rays of energies in the range of a few keV. [...]
arXiv:0706.0637.- 2007 - 13 p. - Published in : Frascati Phys. Ser.: 44 (2007) , pp. 10-113
- Published in : , pp. 101-113 Fulltext: Frasc Phys Ser 44 101 - PDF; arXiv:0706.0637 - PDF; External link: Fulltext
In : 21ème Rencontres de Physique de la Vallée d'Aoste : Results and Perspectives in Particle Physics, La Thuile, Italy, 4 - 10 Mar 2007, pp.101-113
10.
Search for solar axions : the CAST experiment / Andriamonje, Samuel A ; Aune, S ; Barth, K (CERN) ; Belov, A ; Beltrán, B ; Bräuninger, H ; Carmona, J M ; Cebrián, S ; Collar, J I ; Dafni, T (Tech. Univ. Darmstadt ; CERN) et al.
2006 - Published in : AIP Conf. Proc. 878 (2006) 395-401 External link: Published version from AIP
In : 2nd International Conference on the Dark Side of the Universe, Madrid, Spain, 20 - 24 Jun 2006, pp.395-401

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