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1.
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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;
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2.
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EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade
/ Alves Batista, R. (Madrid, IFT) ; Amin, M.A. (Rice U.) ; Barenboim, G. (Valencia U.) ; Bartolo, N. (U. Padua, Dept. Phys. Astron.) ; Baumann, D. (Amsterdam U. ; U. Amsterdam, GRAPPA ; U. Edinburgh, Higgs Ctr. Theor. Phys.) ; Bauswein, A. (Darmstadt, GSI) ; Bellini, E. (Geneva U., Dept. Theor. Phys.) ; Benisty, D. (Cambridge U., DAMTP ; Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; Bertone, G. (Amsterdam U. ; U. Amsterdam, GRAPPA) ; Blasi, P. (GSSI, Aquila ; Gran Sasso) et al.
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. [...]
arXiv:2110.10074.
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134.
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3.
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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
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4.
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Latest results of the CAST axion search
/ Irastorza, I G (DAPNIA, Saclay ; Zaragoza U.) ; Arik, E (Dogus U., Kadikoy) ; Aune, S (DAPNIA, Saclay) ; Autiero, D (CERN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltran, B (Zaragoza U.) ; Borghi, S (CERN) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy) et al.
/CAST
2007 - 9 p.
- Published in : , pp. 301-310
Fulltext: PDF;
In : 42nd Rencontres de Moriond, La Thuile, Italy, 10 - 17 Mar 2007, pp.301-310
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5.
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Solar axion search with the CAST experiment
/ Borghi, S (CERN ; Glasgow U.) ; Arik, E (Dogus U., Kadikoy ; Bogazici U.) ; Aune, S (IRFU, Saclay) ; Autiero, D (CERN ; Lyon, IPN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltrán, B (Zaragoza U.) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy ; Bogazici U.) ; Bräuninger, H (Garching, Max Planck Inst., MPE) et al.
/CAST
The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipe of a LHC prototype dipole. In the phase II, CAST is operating with a buffer gas inside the magnet bore apertures in order to extent the sensitivity of the experiment to larger axion masses. [...]
Paris, France : Moriond, 2008 - 8 p.
- Published in : , pp. 465-472
Fulltext: PDF;
In : 43rd Rencontres de Moriond, La Thuile, Italy, 01 - 08 Mar 2008, pp.465-472
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Physics at the e+ e- Linear Collider
/ Moortgat-Pick, G. (ed.) (Hamburg U. ; DESY) ; Baer, H. (ed.) (Oklahoma U.) ; Battaglia, M. (ed.) (UC, Santa Cruz) ; Belanger, G. (ed.) (Annecy, LAPTH) ; Fujii, K. (ed.) (KEK, Tsukuba) ; Kalinowski, J. (ed.) (Warsaw U.) ; Heinemeyer, S. (ed.) (Cantabria U., Santander) ; Kiyo, Y. (ed.) (Juntendo U.) ; Olive, K. (ed.) (Minnesota U.) ; Simon, F. (ed.) (Munich, Max Planck Inst.) et al.
A comprehensive review of physics at an e+e- Linear Collider in the energy range of sqrt{s}=92 GeV--3 TeV is presented in view of recent and expected LHC results, experiments from low energy as well as astroparticle physics.The report focuses in particular on Higgs boson, Top quark and electroweak precision physics, but also discusses several models of beyond the Standard Model physics such as Supersymmetry, little Higgs models and extra gauge bosons. The connection to cosmology has been analyzed as well..
arXiv:1504.01726; DESY-14-241; CERN-PH-TH-2015-042; FERMILAB-PUB-15-132-T; DESY 14-241; CERN-PH-TH-2015-042.-
Geneva : CERN, 2015-08-14 - 180 p.
- Published in : Eur. Phys. J. C 75 (2015) 371
Article from SCOAP3: PDF; Fulltext: PDF; Springer Open Access article: PDF; External link: Fermilab Library Server (fulltext available)
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7.
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Search for Solar Axions with the CAST-Experiment
/ Vogel, J. (Freiburg U.) ; Arik, E. (Dogus U., Kadikoy) ; Aune, S. (CEA, DSM, Saclay) ; Autiero, D. (CERN) ; Barth, K. (CERN) ; Belov, A. (Moscow, INR) ; Beltran, B. (U. Zaragoza (main)) ; Borghi, S. (CERN) ; Bourlis, G. ; Boydag, F. S. (Dogus U., Kadikoy) et al.
Solar axions can be produced in the Sun via the so-called Primakoff effect. The CERN Axion Solar Telescope (CAST) uses an LHC prototype magnet of about 9 T to reconvert these axions into photons. [...]
2008
- Published in : 10.1142/9789812819093_0049
In : 10th ICATPP Conference on Astroparticle, Particle, Space Physics, Detectors and Medical Physics Applications, Villa Olmo, Como, Italy, 8 - 12 Oct 2007, pp.282-286
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8.
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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
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9.
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Bremsstrahlung gamma rays from light Dark Matter
/ Cirelli, Marco (IPhT, Saclay) ; Serpico, Pasquale D. (Annecy, LAPTH) ; Zaharijas, Gabrijela (ICTP, Trieste)
We discuss the often-neglected role of bremsstrahlung processes on the interstellar gas in computing indirect signatures of Dark Matter (DM) annihilation in the Galaxy, particularly for light DM candidates in the phenomenologically interesting O(10) GeV mass range. Especially from directions close to the Galactic Plane, the expected gamma-ray spectrum is altered via two effects: directly, by the photons emitted in the bremsstrahlung process on the interstellar gas by energetic electrons which are among the DM annihilation byproducts; indirectly, by the modification of the same electron spectrum, due to the additional energy loss process in the diffusion-loss equation (e.g. [...]
arXiv:1307.7152; CERN-PH-TH-2012-171; SACLAY-T12-048; LAPTH-038-13; CERN-PH-TH-2012-171; SACLAY-T12-048; LAPTH-038-13.-
2013-11-13 - 17 p.
- Published in : JCAP 11 (2013) 035
External link: Preprint
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10.
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Gamma ray constraints on Decaying Dark Matter
/ Cirelli, Marco (CERN ; Saclay) ; Moulin, Emmanuel (Saclay) ; Panci, Paolo (Southern Denmark U., CP3-Origins) ; Serpico, Pasquale D. (Annecy, LAPTH ; CERN) ; Viana, Aion (Saclay)
We derive new bounds on decaying Dark Matter from the gamma ray measurements of (i) the isotropic residual (extragalactic) background by Fermi and (ii) the Fornax galaxy cluster by HESS. We find that those from (i) are among the most stringent constraints currently available, for a large range of DM masses and a variety of decay modes, excluding half-lives up to ~10^26 to few 10^27 seconds. [...]
CERN-PH-TH-2012-110; SACLAY-T12-034; IRFU-12-34; DIAS-2012-11; LAPTH-023-12; arXiv:1205.5283; SACLAY--T12-034; CP3-ORIGINS-2012-10; CERN-PH-TH-2012-110; SACLAY-T12-034; IRFU-12-34; CP3-ORIGINS-2012-10; DIAS-2012-11; LAPTH-023-12.-
2012 - 18 p.
- Published in : Phys. Rev. D 86 (2012) 083506
APS Published version, local copy: PDF; Preprint: PDF; External link: Preprint
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