0000000000190449

AUTHOR

C. Fiorini

showing 2 related works from this author

Searches for lepton number violation and resonances in K± → πμμ decays

2017

The NA48/2 experiment at CERN collected a large sample of charged kaon decays to final states with multiple charged particles in 2003–2004. A new upper limit on the rate of the lepton number violating decay K±→π∓μ±μ± is reported: B(K±→π∓μ±μ±)<8.6×10−11 at 90% CL. Searches for two-body resonances X in K±→πμμ decays (such as heavy neutral leptons N4 and inflatons χ ) are also presented. In the absence of signals, upper limits are set on the products of branching fractions B(K±→μ±N4)B(N4→πμ) and B(K±→π±X)B(X→μ+μ−) for ranges of assumed resonance masses and lifetimes. The limits are in the (10−11,10−9) range for resonance lifetimes below 100 ps.

leptonBEAM01 natural sciences7. Clean energyPhysics Particles & FieldsHigh Energy Physics - ExperimentLIMITSkaon physicsCERNIntermediate statelepton number violation neutrinos dark matter kaon physicsPhysicsVMSMLarge Hadron ColliderPhysicsCharge KaonsneutrinosNuclear and High Energy Physics; CERN; leptonsHigh Energy Physics - Experiment; Charge Kaons; Lepton number violationNuclear & Particles PhysicsCharged particlelcsh:QC1-999NEUTRAL HEAVY-LEPTONSPhysics Nuclearlepton number violationPhysical SciencesParticle physicsNuclear and High Energy Physicsleptonskaon decays lepton number violationNuclear and High Energy Physics lepton kaon meson lepton number violation NA48Socio-culturaleAstronomy & AstrophysicsUPPER-BOUNDSdark matterNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciencesDARK-MATTERPARTICLES010306 general physicsScience & Technologykaon decays010308 nuclear & particles physicsBranching fractionResonanceInflatonLepton numberkaon mesonNA48High Energy Physics::Experimentlcsh:PhysicsLepton
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The NHXM observatory

2011

Exploration of the X-ray sky has established X-ray astronomy as a fundamental astrophysical discipline. While our knowledge of the sky below 10 keV has increased dramatically (∼8 orders of magnitude) by use of grazing incidence optics, we still await a similar improvement above 10 keV, where to date only collimated instruments have been used. Also ripe for exploration is the field of X-ray polarimetry, an unused fundamental tool to understand the physics and morphology of X-ray sources. Here we present a novel mission, the New Hard X-ray Mission (NHXM) that brings together for the first time simultaneous high-sensitivity, hard-X-ray imaging, broadband spectroscopy and polarimetry. NHXM will…

Black-holesAcceleration mechanismCosmic Visionmedia_common.quotation_subjectPolarimetry7. Clean energy01 natural sciencesMissionsCosmologyPhysical cosmologyNon-thermal emissionAcceleration mechanism; Accretion physics; Black-holes; Compact objects; Cosmology; Missions; Non-thermal emission; X-ray imaging; X-ray polarimetry; Astronomy and Astrophysics; Space and Planetary ScienceObservatory0103 physical sciencesBroadbandX-ray polarimetry010303 astronomy & astrophysicsCompact objectsmedia_commonPhysics010308 nuclear & particles physicsX-ray imagingVegaAstronomyAstronomy and AstrophysicsAccretion physicsCosmologySkySpace and Planetary ScienceExperimental Astronomy
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