6533b857fe1ef96bd12b3c83

RESEARCH PRODUCT

Reliability of Monte Carlo event generators for gamma-ray dark matter searches

A. De La Cruz-dombrizA. De La Cruz-dombrizAntonio L. MarotoJose A. R. CembranosRoberto A. LinerosViviana Gammaldi

subject

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FortranMonte Carlo methodDark matterFOS: Physical sciencesGamma ray spectra01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Reliability (semiconductor)0103 physical sciences010303 astronomy & astrophysicsEvent generatorcomputer.programming_languageHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGamma rayFísicaHigh Energy Physics - PhenomenologyMonte Carlo SimulationsAstrophysics - High Energy Astrophysical PhenomenacomputerEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics

description

We study the differences in the gamma-ray spectra simulated by four Monte Carlo event generator packages developed in particle physics. Two different versions of PYTHIA and two of HERWIG are analyzed, namely PYTHIA 6.418 and HERWIG 6.5.10 in Fortran and PYTHIA 8.165 and HERWIG 2.6.1 in C++. For all the studied channels, the intrinsic differences between them are shown to be significative and may play an important role in misunderstanding dark matter signals.

10.1007/jhep09(2013)077http://eprints.ucm.es/25976/