0000000000123262

AUTHOR

Mattias Blennow

showing 5 related works from this author

Summary Report of MINSIS Workshop in Madrid

2010

Recent developments on tau detection technologies and the construction of high intensity neutrino beams open the possibility of a high precision search for non-standard {\mu} - {\tau} flavour transition with neutrinos at short distances. The MINSIS - Main Injector Non-Standard Interaction Search- is a proposal under discussion to realize such precision measurement. This document contains the proceedings of the workshop which took place on 10-11 December 2009 in Madrid to discuss both the physics reach as well as the experimental requirements for this proposal.

High Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)FOS: Physical sciencesHigh Energy Physics - ExperimentParticle Physics - Phenomenology
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Neutrino probes of the nature of light dark matter

2011

Dark matter particles gravitationally trapped inside the Sun may annihilate into Standard Model particles, producing a flux of neutrinos. The prospects of detecting these neutrinos in future multi-\kton{} neutrino detectors designed for other physics searches are explored here. We study the capabilities of a 34/100 \kton{} liquid argon detector and a 100 \kton{} magnetized iron calorimeter detector. These detectors are expected to determine the energy and the direction of the incoming neutrino with unprecedented precision allowing for tests of the dark matter nature at very low dark matter masses, in the range of 5-50 GeV. By suppressing the atmospheric background with angular cuts, these t…

Physics::Instrumentation and DetectorsDark matterFOS: Physical sciences01 natural sciences7. Clean energyStandard ModelNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsLight dark matterParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAnnihilationCalorimeter (particle physics)010308 nuclear & particles physicsDetectorFísicaAstronomy and AstrophysicsHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Aidnogenesis via Leptogenesis and Dark Sphalerons

2010

We discuss aidnogenesis, the generation of a dark matter asymmetry via new sphaleron processes associated to an extra non-abelian gauge symmetry common to both the visible and the dark sectors. Such a theory can naturally produce an abundance of asymmetric dark matter which is of the same size as the lepton and baryon asymmetries, as suggested by the similar sizes of the observed baryonic and dark matter energy content, and provide a definite prediction for the mass of the dark matter particle. We discuss in detail a minimal realization in which the Standard Model is only extended by dark matter fermions which form "dark baryons" through an SU(3) interaction, and a (broken) horizontal symme…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsAsymmetrySphaleronStandard ModelDark matter haloBaryonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)LeptogenesisAnomaly (physics)Astrophysics - High Energy Astrophysical Phenomenamedia_common
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Gain fractions of future neutrino oscillation facilities over T2K and NOvA

2013

We evaluate the probability of future neutrino oscillation facilities to discover leptonic CP violation and/or measure the neutrino mass hierarchy. We study how this probability is affected by positive or negative hints for these observables to be found at T2K and NO nu A. We consider the following facilities: LBNE; T2HK; and the 10 GeV Neutrino Factory (NF10), and show how their discovery probabilities change with the running time of T2K and NO nu A conditioned to their results. We find that, if after 15 years T2K and NO nu A have not observed a 90% CL hint of CP violation, then LBNE and T2HK have less than a 10% chance of achieving a 5 sigma discovery, whereas NF10 still has a similar to …

NOνAPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentRunning timeHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)CP violationHigh Energy Physics - Phenomenology (hep-ph)Physical Sciences0103 physical sciencesFysikCP violationNeutrino PhysicsNeutrino FactoryFermilabNeutrino010306 general physicsNeutrino oscillationJournal of High Energy Physics
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Asymmetric Dark Matter and Dark Radiation

2012

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and generally related, thus predicting DM masses around 5 GeV in order to obtain the correct density. The main challenge for successful models is to ensure efficient annihilation of the thermally produced symmetric component of such a light DM candidate without violating constraints from collider or direct searches. A common way to overcome this involves a light mediator, into which DM can efficiently annihilate and which subsequently decays into Standard Mod…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundDark matterFOS: Physical sciences01 natural sciencesStandard Modelsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanck010306 general physicsParticle Physics - Phenomenologymedia_commonPhysicsCosmologia010308 nuclear & particles physicsMatter power spectrumAstronomy and AstrophysicsUniverseBaryonHigh Energy Physics - Phenomenology13. Climate actionDark radiationsymbolsAstrophysics - Cosmology and Nongalactic Astrophysics
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