0000000000355732

AUTHOR

Bz

showing 2 related works from this author

Measurement of matter-antimatter differences in beauty baryon decays

2017

Differences in the behaviour of matter and antimatter have been observed in $K$ and $B$ meson decays, but not yet in any baryon decay. Such differences are associated with the non-invariance of fundamental interactions under the combined charge-conjugation and parity transformations, known as $C\!P$ violation. Using data from the LHCb experiment at the Large Hadron Collider, a search is made for $C\!P$-violating asymmetries in the decay angle distributions of $\Lambda^0_b$ baryons decaying to $p\pi^-\pi^+\pi^-$ and $p\pi^-K^+K^-$ final states. These four-body hadronic decays are a promising place to search for sources of $C\!P$ violation both within and beyond the Standard Model of particle…

Physics beyond the Standard ModelHadrontransformation [parity]General Physics and Astronomy7000 GeV-cms8000 GeV-cmsviolation [CP]decay [meson]01 natural sciencesHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - Experiment (hep-ex)antimatterscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]AntimatèriaDecays of bottom mesons Flavor symmetriesB mesonLHCb - Abteilung HintonPhysicsLarge Hadron Collider02 Physical Sciencesnew physicsCabibbo–Kobayashi–Maskawa matrixPhysicsparity: transformationParticle physicsFlavor symmetriesCharge conjugation parity time reversal and other discrete symmetrieDecays of bottom mesonsasymmetry: CPCERN LHC CollCP-VIOLATION; LAMBDA(B)meson: decayangular distribution [decay]AntimatterPhysical SciencesCP violationLHCcolliding beams [p p]Lambda/b0: hadronic decayParticle Physics - Experimentp p: scatteringParticle physicsAntimatterFluids & PlasmasPhysics MultidisciplinaryLambda/b0 --> p pi- K+ K-FOS: Physical scienceshadronic decay [Lambda/b0]Lambda/b0 --> p pi+ 2pi-CP [asymmetry]530Lambda/b0 --> p pi+ 2pi-Determination of Cabibbo-Kobayashi & Maskawa (CKM) matrix elementNONuclear physicsPhysics and Astronomy (all)LAMBDA(B)TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesCP: violationdecay: angular distributionddc:530010306 general physicsLarge Hadron Collider (France and Switzerland)01 Mathematical SciencesScience & Technologycharge conjugation010308 nuclear & particles physicshep-exLambda/b0 --> p pi- K+ K-High Energy Physics::PhenomenologyGran Col·lisionador d'HadronsLHC-BHEPBaryonLHCbCP-VIOLATIONCKM matrixHadronic decays of baryonBottom baryons (|B|>0)High Energy Physics::ExperimentFísica de partículesExperimentsp p: colliding beamsstatisticalexperimental results
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Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

2009

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhotonAstronomyFOS: Physical sciencesFluxCosmic rayFotonesAstrophysicsEXTENSIVE AIR-SHOWERS01 natural sciences7. Clean energyNuclear physicsCascada atmosféricaUltra high energy (UHE)0103 physical sciencesLimit (mathematics)FLUORESCENCEUltra-high energy cosmic ray010303 astronomy & astrophysicsDETECTORCosmic raysCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysics010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomy and AstrophysicsPierre Auger ObservatoryPROFILESRadiación cósmicaPhotonLongitudinal development13. Climate actionphoton fractionComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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