CERN Accelerating science

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1.
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.
- 134.
Fulltext
2.
Searches for gamma-ray lines and `pure WIMP' spectra from Dark Matter annihilations in dwarf galaxies with H.E.S.S / H.E.S.S. Collaboration
Dwarf spheroidal galaxies are among the most promising targets for detecting signals of Dark Matter (DM) annihilations. The H.E.S.S. [...]
arXiv:1810.00995; DESY 18-157; DESY-18-157; CERN-TH-2018-201.- 2018-11-23 - 23 p. - Published in : JCAP 11 (2018) 037 Fulltext: PDF;
3.
Science with the Cherenkov Telescope Array / Cherenkov Telescope Array Consortium Collaboration
The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. [...]
arXiv:1709.07997.
- 2017. - 211 p.
Preprint
4.
On cosmic-ray self-generated turbulence of supernova remnant shocks / Marcowith, A
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.221 (v.3)
5.
Non stationary pair model in blazar / Marcowith, A ; Henri, G ; Renaud, N
2000
In : 4th Integral Workshop : Exploring the Gamma-Ray Universe, Alicante, Spain, 4 - 8 Sep 2000, pp.395-398

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142 Marcowith, A
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