Search results for " Space Sciences"

showing 6 items of 26 documents

A new measurement of direct CP violation in the neutral kaon system

1993

A new measurement of the ratio of the CP-violating amplitudes for $K_{L} \to 2\pi^{0}$ and $K_{L} \to \pi^{+}\pi^{-}$ is reported. The measured value for $\Re = |\eta_{00} / \eta_{ +-}|^{2}$ is $0.9878 \pm 0.0026 \pm 0.0030$, where the first error is the statistical uncertainty and the second is the estimate of the systematic uncertainty. This gives a value for the parameter describing direct CP violation: $\Re$ $\epsilon'/\epsilon = (2.0 \pm 0.7) \times 10^{−3}$ .

Systematic errorPhysicsNuclear and High Energy PhysicsParticle physicsValue (computer science)NA48 experimentMolecularElementary particleAtomicNuclear & Particles PhysicsNuclear physicsAmplitudeParticle and Plasma PhysicsEnergy spectrumCP violationNuclearNeutral particleMathematical PhysicsAstronomical and Space SciencesParticle Physics - Experiment
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The 30 Year Search for the Compact Object in SN 1987A

2018

Despite more than 30 years of searches, the compact object in Supernova (SN) 1987A has not yet been detected. We present new limits on the compact object in SN 1987A using millimeter, near-infrared, optical, ultraviolet, and X-ray observations from ALMA, VLT, HST, and Chandra. The limits are approximately 0.1 mJy ($0.1\times 10^{-26}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) at 213 GHz, 1 Lsun ($6\times 10^{-29}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in optical if our line-of-sight is free of ejecta dust, and $10^{36}$ erg s$^{-1}$ ($2\times 10^{-30}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$) in 2-10 keV X-rays. Our X-ray limits are an order of magnitude less constraining than previous limits because we use a…

[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstrophysicsPhysical Chemistry01 natural sciences7. Clean energyAtomicLuminosityParticle and Plasma PhysicsQB460Astrophysics::Solar and Stellar AstrophysicsAbsorption (logic)10. No inequality010303 astronomy & astrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEAccretion (meteorology)SUPERNOVA REMNANT 1987ASupernovaAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesPhysical Chemistry (incl. Structural)NEUTRON-STARSCIRCUMSTELLAR RINGX-RAYSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBLUE SUPERGIANTSAstrophysics::Cosmology and Extragalactic AstrophysicsCompact starAstronomy & Astrophysicsstars: neutronneutron [stars]Pulsarindividual [supernovae]0103 physical sciencesblack holes [stars]NuclearINTEGRAL FIELD SPECTROSCOPY010306 general physicsUNDERGROUND SCINTILLATION TELESCOPEsupernovae: individualAstrophysics::Galaxy AstrophysicsOrganic ChemistryMolecularAstronomy and AstrophysicsHUBBLE-SPACE-TELESCOPEEffective temperatureNeutron starRAY EMISSION-LINESPhysics and Astronomyindividual (SN 1987A) [supernovae]13. Climate actionSpace and Planetary ScienceLARGE-MAGELLANIC-CLOUD[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]stars: black holes
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Overview paper: New insights into aerosol and climate in the Arctic

2019

Motivated by the need to predict how the Arctic atmosphere will change in a warming world, this article summarizes recent advances made by the research consortium NETCARE (Network on Climate and Aerosols: Addressing Key Uncertainties in Remote Canadian Environments) that contribute to our fundamental understanding of Arctic aerosol particles as they relate to climate forcing. The overall goal of NETCARE research has been to use an interdisciplinary approach encompassing extensive field observations and a range of chemical transport, earth system, and biogeochemical models. Several major findings and advances have emerged from NETCARE since its formation in 2013. (1) Unexpectedly high summer…

[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Arctic hazeAtmospheric Science010504 meteorology & atmospheric sciencesGlobal warmingClimate change010501 environmental sciencesMineral dustAtmospheric sciences01 natural sciencesSea surface microlayerlcsh:QC1-999Atmospheric SciencesAerosollcsh:ChemistryClimate ActionDeposition (aerosol physics)lcsh:QD1-999Arctic[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology13. Climate actionMeteorology & Atmospheric Scienceslcsh:PhysicsAstronomical and Space Sciences0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection

2020

Predicting the large-scale eruptions from the solar corona and their propagation through interplanetary space remains an outstanding challenge in solar- and helio-physics research. In this article, we describe three dimensional magnetohydrodynamic simulations of the inner heliosphere leading up to and including the extreme interplanetary coronal mass ejection (ICME) of 23 July 2012, developed using the code PLUTO. The simulations are driven using the output of coronal models for Carrington rotations 2125 and 2126 and, given the uncertainties in the initial conditions, are able to reproduce an event of comparable magnitude to the 23 July ICME, with similar velocity and density profiles at 1 …

astro-ph.SRSpace weather010504 meteorology & atmospheric sciencesMHDSolar windSTORMFOS: Physical sciencesMagnitude (mathematics)Context (language use)PROPAGATIONAstronomy & AstrophysicsDisturbancesSpace weatherPROTON01 natural sciencesEVENTSMagnetohydrodynamicsPhysics - Space Physicsphysics.plasm-ph0201 Astronomical and Space Sciences0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologySUNAstronomy and AstrophysicsARRIVALGeophysicsEVOLUTIONSpace Physics (physics.space-ph)Physics - Plasma PhysicsPlasma Physics (physics.plasm-ph)PlutoSolar windAstrophysics - Solar and Stellar Astrophysicsphysics.space-ph13. Climate actionSpace and Planetary ScienceDragPhysical Sciencesastro-ph.EPMagnetohydrodynamicsInterplanetary coronal mass ejectionsHeliosphereAstrophysics - Earth and Planetary AstrophysicsSolar Physics
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Global analysis of the pMSSM in light of the Fermi GeV excess: prospects for the LHC Run-II and astroparticle experiments

2016

We present a new global fit of the 19-dimensional phenomenological Minimal Supersymmetric Standard Model (pMSSM-19) that comply with all the latest experimental results from dark matter indirect, direct and accelerator dark matter searches. We show that the model provides a satisfactory explanation of the excess of gamma-rays from the Galactic centre observed by the Fermi~Large Area Telescope, assuming that it is produced by the annihilation of neutralinos in the Milky Way halo. We identify two regions that pass all the constraints: the first corresponds to neutralinos with a mass ~80-100 GeV annihilating into WW with a branching ratio of 95% ; the second to heavier neutralinos, with mass ~…

supersymmetry and cosmologyParticle physicsMilky WayAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesgamma ray experiments7. Clean energy01 natural sciences0202 Atomic Molecular Nuclear Particle And Plasma PhysicsHigh Energy Physics - Phenomenology (hep-ph)Settore FIS/05 - Astronomia e Astrofisica0103 physical sciencesHigh Energy Physics010306 general physicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)PhysicsAnnihilationLarge Hadron Colliderdark matter detectorsdark matter theory010308 nuclear & particles physicsBranching fractionHigh Energy Physics::Phenomenologyhep-phAstronomy and AstrophysicsNuclear & Particles Physics0201 Astronomical And Space SciencesHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentHaloFermi Gamma-ray Space TelescopeMinimal Supersymmetric Standard Model
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Recommendations of the LHC Dark Matter Working Group: Comparing LHC searches for dark matter mediators in visible and invisible decay channels and ca…

2019

Physics of the Dark Universe 26, 100377 (2019). doi:10.1016/j.dark.2019.100377

transverse momentum: missing-energyscale: TeVAtomic01 natural sciencesParticle and Plasma Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]TeV [scale]010303 astronomy & astrophysicsPhysicsLarge Hadron ColliderCMSPhysicsaxial-vectorMonte Carlo [numerical calculations]ATLASCERN LHC Collinterpretation of experimentsrelic density [dark matter]colliding beams [p p]numerical calculations: Monte CarloAstronomical and Space SciencessignatureParticle physicsp p: scatteringDark matterlepton: couplingdark matter: production5300103 physical sciencesThermalNuclearddc:530Pseudovector010308 nuclear & particles physicsdark matter: relic densityMolecularAstronomy and Astrophysicsmediation [dark matter]dark matter: mediationproduction [dark matter]Space and Planetary Sciencemissing-energy [transverse momentum][PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]invisible decaycoupling [lepton][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]p p: colliding beamsvectorLeptonexperimental results
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