Search results for "matter [quantum chromodynamics]"

showing 10 items of 162 documents

Shining primordial black holes

2021

We study the well-motivated mixed dark matter (DM) scenario composed of a dominant thermal WIMP, highlighting the case of $SU(2)_L$ triplet fermion "winos", with a small fraction of primordial black holes (PBHs). After the wino kinetic decoupling, the DM particles are captured by PBHs leading to the presence of PBHs with dark minihalos in the Milky Way today. The strongest constraints for the wino DM come from the production of narrow line gamma rays from wino annihilation in the Galactic Center. We analyse in detail the viability of the mixed wino DM scenario, and determine the constraints on the fraction of DM in PBHs assuming a cored halo profile in the Milky Way. We show that already wi…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Milky WayAstrophysics::High Energy Astrophysical PhenomenaastrofysiikkaDARK-MATTER ANNIHILATIONFOS: Physical sciencesmustat aukotPrimordial black holeAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicskosmologia7. Clean energy01 natural sciences114 Physical sciencesGeneral Relativity and Quantum Cosmologypimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Annihilation010308 nuclear & particles physicsGalactic CenterGAMMA-RAYSCONSTRAINTSFermionHigh Energy Physics - PhenomenologyMixed dark matterMILKYHaloAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Searching for sterile neutrino with X-ray intensity mapping

2019

The cosmological X-ray emission associated to the possible radiative decay of sterile neutrinos is composed by a collection of lines at different energies. For a given mass, each line corresponds to a given redshift. In this work, we cross correlate such line emission with catalogs of galaxies tracing the dark matter distribution at different redshifts. We derive observational prospects by correlating the X-ray sky that will be probed by the eROSITA and Athena missions with current and near future photometric and spectroscopic galaxy surveys. A relevant and unexplored fraction of the parameter space of sterile neutrinos can be probed by this technique.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)X-ray telescopes; dark matter experiments; dark matter theory; power spectrumdark matter theoryAstrophysics::High Energy Astrophysical Phenomenadark matter experimentsAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicspower spectrumHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsX-ray telescopes
researchProduct

Despicable dark relics: generated by gravity with unconstrained masses

2019

We demonstrate the existence of a generic, efficient and purely gravitational channel producing a significant abundance of dark relics during reheating after the end of inflation. The mechanism is present for any inert scalar with the non-minimal curvature coupling $\xi R\chi^2$ and the relic production is efficient for natural values $\xi = {\cal O}(1)$. The observed dark matter abundance can be reached for a broad range of relic masses extending from $m \sim 1 {\rm k eV}$ to $m \sim 10^{8} {\rm GeV}$, depending on the scale of inflation and the dark sector couplings. Frustratingly, such relics escape direct, indirect and collider searches since no non-gravitational couplings to visible ma…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)inationScalar (mathematics)Dark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCurvature01 natural sciencesGeneral Relativity and Quantum Cosmologylaw.inventionpimeä aineGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesinflationColliderkosminen inflaatioPhysicsInflation (cosmology)Couplingdark matter theory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSCALAR-FIELD115 Astronomy Space science16. Peace & justicequantum field theory on curved spaceHigh Energy Physics - PhenomenologyProduction (computer science)kvanttikenttäteoriaMATTERAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
researchProduct

Design of New Resonant Haloscopes in the Search for the Dark Matter Axion: A Review of the First Steps in the RADES Collaboration

2022

This article belongs to the Special Issue Studying the Universe from Spain.

Dark matter detectorsResonant cavitiesaxionsdark matter detectorsPhysics - Instrumentation and Detectorshep-exAxionsGeneral Physics and AstronomyFOS: Physical sciencesElementary particle physicsInstrumentation and Detectors (physics.ins-det)QC793-793.5HaloscopesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)haloscopesDetectors and Experimental Techniquesphysics.ins-detParticle Physics - Experimentresonant cavities
researchProduct

Search for Subsolar Mass Ultracompact Binaries in Advanced LIGO's Second Observing Run

2019

We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO’s second observing run. In contrast to a previous search of Advanced LIGO data from the first observing run, this search includes the effects of component spin on the gravitational waveform. We identify no viable gravitational-wave candidates consistent with subsolar mass ultracompact binaries with at least one component between \ud0.2\ud \ud \udM\ud⊙\ud–\ud1.0\ud \ud \udM\ud⊙\ud. We use the null result to constrain the binary merger rate of (\ud0.2\ud \ud \udM\ud⊙\ud, \ud0.2\ud \ud \udM\ud⊙\ud) binaries to be less than \ud3.7\ud×\ud10\ud5\ud \ud \udGpc\ud−\ud3\ud \udyr\ud−\ud1\udand the binary …

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenbinary: massAstrofísicaGravitacióFormation modeldensity: fluctuationAstronomyGeneral Physics and Astronomydetector: networkspin01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSblack hole: formationddc:550black holeDark MatterAstrophysics::Solar and Stellar AstrophysicsLIGOQCQBnucleus: interactionSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational wave; physics; astronomyPhysicsarticleDensity fluctuationgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]astro-ph.COAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenablack hole: primordialGravitationAstrophysics - Cosmology and Nongalactic AstrophysicsMatter densitydensity: primordialCosmology and Nongalactic Astrophysics (astro-ph.CO)coolinggr-qcAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinaryCooling mechanismPrimordial black holesFOS: Physical sciencesdark matter: densityGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesNuclear interactionGravitation and AstrophysicsMergingGeneral Relativity and Quantum Cosmologynull resultSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technologymass: solarCosmologiaStellar evolutions010308 nuclear & particles physicsMatter fractionsgravitational radiationRCUKblack hole: massGalaxiesbinary: compactStarsgravitational radiation detectordetector: sensitivityVIRGOPhysics and Astronomygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Gravitational waves Black holes (astronomy) Gravitational self forcePhysical Review Letters
researchProduct

GW170817: Measurements of Neutron Star Radii and Equation of State

2018

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESGW170817BINARIESddc:550DENSELIGODENSE MATTEREquation of State010303 astronomy & astrophysicsQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsNeutron Star RadiusPhysicsGravitational effectsEquations of stateParametrizationsElectromagnetic observationsGravitational-wave signals3. Good healthQUADRUPOLE-MOMENTSMacroscopic propertiesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEquations of state of nuclear matterGravitational wavesaturation: densityBinary neutron starsNUCLEON MATTEREquations of state of nuclear matter; Gravitational wave sources; Gravitational waves; Nuclear matter in neutron starsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaGW170817 Neutron Star Radius Equation of StatePhysics Multidisciplinaryneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionGravitation and AstrophysicsNuclear matter in neutron starsGravitational waveselectromagnetic field: productionPhysics and Astronomy (all)Pulsargalaxy: binary0103 physical sciencesddc:530NeutronMASSESSTFCequation of state: parametrizationAstrophysics::Galaxy AstrophysicsNeutronsExtreme conditionsGravitational wave sourcesEquation of stateScience & TechnologyNeutron Star Interior Composition Explorer010308 nuclear & particles physicsGravitational wavegravitational radiationRCUKFlocculationSaturation densityUNIVERSAL RELATIONSStarsLIGOgravitational radiation detectorNeutron starStarsVIRGOPhysics and Astronomygravitational radiation: emissionneutron star: binary: coalescenceDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]MATTER
researchProduct

Electroluminescence TPCs at the thermal diffusion limit

2019

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

ElectroluminiscènciaNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsDark Matter and Double Beta DecayFOS: Physical scienceschemistry.chemical_elementElectronAtomic01 natural sciences7. Clean energyMathematical SciencesHigh Energy Physics - ExperimentTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)Particle and Plasma PhysicsXenonIonization0103 physical sciencesDark Matter and Double Beta Decay (experiments)Nuclearlcsh:Nuclear and particle physics. Atomic energy. RadioactivityDiffusion (business)010306 general physicsMathematical PhysicsPhysicsQuantum Physics010308 nuclear & particles physicsResolution (electron density)MolecularFísicaNuclear energyInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsParticle correlations and fluctuations85-05ElectroluminescencechemistryRare decayYield (chemistry)Photon productionPhysical SciencesScintillation counterEnergia nuclearlcsh:QC770-798Atomic physicsEnergy (signal processing)
researchProduct

Analytical wave function of an atom in the presence of a laser pulse

2005

We study a simple model atom that has two bound states and a continuum of free states, interacting with a strong electromagnetic field. In our analysis we assume that only the continuum-continuum transitions occur- ring between degenerate free states are important for the dynamics of the atomic system; adopting this sim- plifying hypothesis, we show that it is possible to describe the time evolution of the atom by means of an infinite but discrete set of first-order differential equations describing a formal model atom that has two bound states and a degenerate quasicontinuum of states. Moreover, these equations depend on a small number of parameters of the bare atom and of the external las…

Electromagnetic fieldPhysicsDifferential equationDegenerate energy levelsTime evolutionAtomic and Molecular Physics and OpticsAtom laserQuantum mechanicsAtomBound stateLaser matter interactionPhysics::Atomic PhysicsAtomic physicsWave function
researchProduct

Photosensitivity of SiO2–Al and SiO2–Na glasses under ArF (193 nm) laser

2009

Abstract Photosensitivity of SiO 2 –Al and SiO 2 –Na glass samples was probed by means of the induced optical absorption and luminescence as well as by electron spin-resonance (ESR) after irradiation with excimer-laser photons (ArF, 193 nm). Permanent visible darkening in the case of SiO 2 –Al and transient, life time about one hour, visible darkening in the case of SiO 2 –Na was found under irradiation at 290 K. No darkening was observed at 80 K for either kind of material. This investigation is dedicated to revealing the electronic processes responsible for photosensitivity at 290 and 80 K. The photosensitivity of both materials is related to impurity defects excited directly in the case …

Electron mobilityPhotoluminescenceChemistryDopingAnalytical chemistryCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsPhotosensitivityImpurityMaterials ChemistryCeramics and CompositesIrradiationRadiation effects Glasses Laser–matter interactions Optical spectroscopy Defects Optical properties Absorption Lasers Luminescence Photoinduced effects Time resolved measurements Oxide glasses Alkali silicates Aluminosilicates Silica Silicates Radiation Electron spin resonanceSpectroscopyLuminescence
researchProduct

Stable isotope and fatty acid analysis reveal the ability of sea cucumbers to use fish farm waste in integrated multi-trophic aquaculture

2022

Stable isotope ratios, carbon (δ13C) and nitrogen (δ15N), and fatty acids validated the trophic connection between farmed fish in a commercial nearshore fish farm and sea cucumbers in the Mediterranean Sea. This dual tracer approach evaluated organic matter transfer in integrated multi-trophic aquaculture (IMTA) and the ability of sea cucumbers to incorporate fish farm waste (fish faeces and uneaten artificial fish feed) into their tissue. Between October 2018 and September 2019, Holothuria (Roweothuria) poli Delle Chiaje, 1824, co-cultured at IMTA sites directly below one of the commercial fish cage , at 10 m and 25 m from the selected fish cage, and at two reference sites over 800 m from …

Environmental EngineeringStable isotopes Fatty acids Sea cucumbers Integrated multi-trophic aquaculture Organic matter transferIsotopesSea CucumbersFatty AcidsFisheriesFishesAnimalsGeneral MedicineAquacultureManagement Monitoring Policy and LawWaste Management and Disposal
researchProduct