We correct a few mistakes of the original version of this work (notably related to the computations of extragalactic gamma rays), while at the same time improving and upgrading other aspects (notably as a consequence of the discovery of the higgs boson at the LHC). A brief list of the main changes is:- We include a higgs boson channel hh with mass m(h) = 125 GeV. All previous channels h(m)h(m) are removed.- We correct the formulae for the computation of extragalactic gamma rays (fixing in particular the redshift dependence) as well as the numerical computations (also including a corrected impact of absorption).- We provide a new version of the Optical Depth function, employing updated models of Extragalactic Background Light (EBL) and fixing the redshift dependence.All these corrections and updates are reflected on the numerical ingredients provided on the website;(2) they correspond to Release 2.0.

Erratum: PPPC 4 DM ID: A poor particle physicist cookbook for dark matter indirect detection (Journal of Cosmology and Astroparticle Physics (2012) (1)) / Cirelli M.; Corcella G.; Hektor A.; Hutsi G.; Kadastik M.; Panci P.; Raidal M.; Sala F.; Strumia A.. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - ELETTRONICO. - 2012:10(2012), pp. -2-6. [10.1088/1475-7516/2012/10/E01]

Erratum: PPPC 4 DM ID: A poor particle physicist cookbook for dark matter indirect detection (Journal of Cosmology and Astroparticle Physics (2012) (1))

Sala F.;
2012

Abstract

We correct a few mistakes of the original version of this work (notably related to the computations of extragalactic gamma rays), while at the same time improving and upgrading other aspects (notably as a consequence of the discovery of the higgs boson at the LHC). A brief list of the main changes is:- We include a higgs boson channel hh with mass m(h) = 125 GeV. All previous channels h(m)h(m) are removed.- We correct the formulae for the computation of extragalactic gamma rays (fixing in particular the redshift dependence) as well as the numerical computations (also including a corrected impact of absorption).- We provide a new version of the Optical Depth function, employing updated models of Extragalactic Background Light (EBL) and fixing the redshift dependence.All these corrections and updates are reflected on the numerical ingredients provided on the website;(2) they correspond to Release 2.0.
2012
Erratum: PPPC 4 DM ID: A poor particle physicist cookbook for dark matter indirect detection (Journal of Cosmology and Astroparticle Physics (2012) (1)) / Cirelli M.; Corcella G.; Hektor A.; Hutsi G.; Kadastik M.; Panci P.; Raidal M.; Sala F.; Strumia A.. - In: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. - ISSN 1475-7516. - ELETTRONICO. - 2012:10(2012), pp. -2-6. [10.1088/1475-7516/2012/10/E01]
Cirelli M.; Corcella G.; Hektor A.; Hutsi G.; Kadastik M.; Panci P.; Raidal M.; Sala F.; Strumia A.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/908189
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