Search results for "FOS"

showing 10 items of 15075 documents

PBH assisted search for QCD axion dark matter

2022

The entropy production prior to BBN era is one of ways to prevent QCD axion with the decay constant $F_{a}\in[10^{12}{\rm GeV},10^{16}{\rm GeV}]$ from overclosing the universe when the misalignment angle is $\theta_{\rm i}=\mathcal{O}(1)$. As such, it is necessarily accompanied by an early matter-dominated era (EMD) provided the entropy production is achieved via the decay of a heavy particle. In this work, we consider the possibility of formation of primordial black holes during the EMD era with the assumption of the enhanced primordial scalar perturbation on small scales ($k>10^{4}{\rm Mpc}^{-1}$). In such a scenario, it is expected that PBHs with axion halo accretion develop to ultracomp…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)axionsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmustat aukotAstrophysics::Cosmology and Extragalactic Astrophysicshiukkasfysiikkakosmologianeutron starspimeä aineHigh Energy Physics - Phenomenology (hep-ph)neutronitähdetParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEdark matter experimentsHigh Energy Physics::Phenomenologyprimordial black holesAstronomy and Astrophysicshep-phHigh Energy Physics - Phenomenologyastro-ph.COkvanttiväridynamiikkaHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Dark Sectors and New, Light, Weakly-Coupled Particles

2013

Dark sectors, consisting of new, light, weakly-coupled particles that do not interact with the known strong, weak, or electromagnetic forces, are a particularly compelling possibility for new physics. Nature may contain numerous dark sectors, each with their own beautiful structure, distinct particles, and forces. This review summarizes the physics motivation for dark sectors and the exciting opportunities for experimental exploration. It is the summary of the Intensity Frontier subgroup "New, Light, Weakly-coupled Particles" of the Community Summer Study 2013 (Snowmass). We discuss axions, which solve the strong CP problem and are an excellent dark matter candidate, and their generalizatio…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)hep-exFOS: Physical scienceshep-phAstrophysics::Cosmology and Extragalactic AstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)astro-ph.COParticle Physics - ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsParticle Physics - Phenomenology
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Femtolensing by dark matter revisited

2018

Femtolensing of gamma ray bursts (GRBs) has been put forward as an exciting possibility to probe exotic astrophysical objects with masses below $10^{-13}$ solar masses such as small primordial black holes or ultra-compact dark matter minihalos, made up for instance of QCD axions. In this paper we critically review this idea, properly taking into account the extended nature of the source as well as wave optics effects. We demonstrate that most GRBs are inappropriate for femtolensing searches due to their large sizes. This removes the previous femtolensing bounds on primordial black holes, implying that vast regions of parameter space for primordial black hole dark matter are not robustly con…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)spectraAstrophysics::High Energy Astrophysical PhenomenaDark mattergravitational lensinghaloFOS: Physical sciencesPrimordial black holegamma ray experimentsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsAxionParticle Physics - PhenomenologyPhysicsQuantum chromodynamicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Solar mass010308 nuclear & particles physicsraydark matter experimentsprimordial black holesAstronomy and Astrophysicshep-phPhysical opticsHigh Energy Physics - Phenomenologypair production13. Climate actionastro-ph.COGamma-ray burstlimitsAstrophysics - High Energy Astrophysical Phenomenagravitational-wavesAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Cosmological analogies in the search for new physics in high-energy collisions

2020

In this paper, analogies between multiparticle production in high-energy collisions and the time evolution of the early universe are discussed. A common explanation is put forward under the assumption of an unconventional early state: a rapidly expanding universe before recombination (last scattering surface), followed by the CMB, later evolving up to present days, versus the formation of hidden/dark states in hadronic collisions followed by a conventional QCD parton shower yielding final-state particles. In particular, long-range angular correlations are considered pointing out deep connections between the two physical cases potentially useful for the discovery of new physics.

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciences01 natural sciencesMetric expansion of spaceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment010306 general physicsParton showerParticle Physics - Phenomenologymedia_commonPhysicsQuantum chromodynamics010308 nuclear & particles physicsScatteringTime evolutionhep-phUniverseHigh Energy Physics - Phenomenologyastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Electroweak baryogenesis from a dark sector

2017

Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ lepto…

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)standard model of particle physicsPhysics beyond the Standard ModelSTANDARD MODELFOS: Physical sciences01 natural sciences7. Clean energy114 Physical sciencesdark matterHiggs sectorStandard Modelpimeä aineHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesSINGLET010306 general physicsParticle Physics - PhenomenologyPhysicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalliRADIATIVE NEUTRINO MASShep-phSphaleronBaryogenesisHigh Energy Physics - Phenomenologyastro-ph.COHiggs bosonPHASE-TRANSITIONHigh Energy Physics::ExperimentMATTERAstrophysics - Cosmology and Nongalactic Astrophysics
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Prospects for discovering supersymmetric long-lived particles with MoEDAL

2020

We present a study on the possibility of searching for long-lived supersymmetric partners with the MoEDAL experiment at the LHC. MoEDAL is sensitive to highly ionising objects such as magnetic monopoles or massive (meta)stable electrically charged particles. We focus on prospects of directly detecting long-lived sleptons in a phenomenologically realistic model which involves an intermediate neutral long-lived particle in the decay chain. This scenario is not yet excluded by the current data from ATLAS or CMS, and is compatible with astrophysical constraints. Using Monte Carlo simulation, we compare the sensitivities of MoEDAL versus ATLAS in scenarios where MoEDAL could provide discovery re…

Astrophysics and AstronomyParticle physicsPhysics and Astronomy (miscellaneous)Regular Article - Experimental PhysicsPhysics::Instrumentation and DetectorsMagnetic monopoleFOS: Physical scienceslcsh:AstrophysicsElementary particle01 natural sciencesHigh Energy Physics - ExperimentParticle decayHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityInvariant mass010306 general physicsEngineering (miscellaneous)Particle Physics - Phenomenologyastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Large Hadron Colliderhep-ex010308 nuclear & particles physicsSuperpartnerhep-phSupersymmetryHigh Energy Physics - PhenomenologyMoEDAL experimentlcsh:QC770-798Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentEuropean Physical Journal
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Robust constraint on Lorentz violation using Fermi-LAT gamma-ray burst data

2018

Models of quantum gravity suggest that the vacuum should be regarded as a medium with quantum structure that may have non-trivial effects on photon propagation, including the violation of Lorentz invariance. Fermi Large Area Telescope (LAT) observations of gamma-ray bursts (GRBs) are sensitive probes of Lorentz invariance, via studies of energy-dependent timing shifts in their rapidly-varying photon emissions. In this paper we analyze the Fermi-LAT measurements of high-energy gamma rays from GRBs with known redshifts, allowing for the possibility of energy-dependent variations in emission times at the sources as well as a possible non-trivial refractive index in vacuo for photons. We use st…

Astrophysics and AstronomyPhotongr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSensitivity (control systems)010306 general physicsParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGeneral Relativity and CosmologyGamma rayhep-phRedshiftHigh Energy Physics - PhenomenologyAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstEnergy (signal processing)Fermi Gamma-ray Space Telescope
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High magnetic fields for fundamental physics

2018

Various fundamental-physics experiments such as measurement of the birefringence of the vacuum, searches for ultralight dark matter (e.g., axions), and precision spectroscopy of complex systems (including exotic atoms containing antimatter constituents) are enabled by high-field magnets. We give an overview of current and future experiments and discuss the state-of-the-art DC- and pulsed-magnet technologies and prospects for future developments.

Astrophysics and AstronomyPhysics - Instrumentation and Detectorsmagnet: designmagnetic field: highAtomic Physics (physics.atom-ph)AxionsDark matterComplex systemOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesphysics.atom-phNOPhysics - Atomic PhysicsNuclear physicsPhysics and Astronomy (all)Neutrino mass0103 physical sciencesDark matter[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Axions; Dark matter; High-field magnets; Neutrino mass; Spectroscopy; Vacuum birefringence; Physics and Astronomy (all)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Axionphysics.ins-detSpectroscopyactivity reportExotic atomPhysicsVacuum birefringence010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Polarization (waves)magnet: technology[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]3. Good healthMagnetic fieldHigh-field magnetsAntimatterMagnetAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background

2020

Sterile neutrinos with mass in the eV-scale and large mixings of order $\theta_0\simeq 0.1$ could explain some anomalies found in short-baseline neutrino oscillation data. Here, we revisit a neutrino portal scenario in which eV-scale sterile neutrinos have self-interactions via a new gauge vector boson $\phi$. Their production in the early Universe via mixing with active neutrinos can be suppressed by the induced effective potential in the sterile sector. We study how different cosmological observations can constrain this model, in terms of the mass of the new gauge boson, $M_\phi$, and its coupling to sterile neutrinos, $g_s$. Then, we explore how to probe part of the allowed parameter spa…

Astrophysics and AstronomySterile neutrinoParticle physicsScale (ratio)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesNeutrino oscillation010303 astronomy & astrophysicsParticle Physics - Phenomenologymedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gauge boson010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyhep-phAstronomy and AstrophysicsUniverse3. Good healthSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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The ALHAMBRA survey: Accurate merger fractions by PDF analysis of photometric close pairs

2014

Our goal is to develop and test a novel methodology to compute accurate close pair fractions with photometric redshifts. We improve the current methodologies to estimate the merger fraction f_m from photometric redshifts by (i) using the full probability distribution functions (PDFs) of the sources in redshift space, (ii) including the variation in the luminosity of the sources with z in both the selection of the samples and in the luminosity ratio constrain, and (iii) splitting individual PDFs into red and blue spectral templates to deal robustly with colour selections. We test the performance of our new methodology with the PDFs provided by the ALHAMBRA photometric survey. The merger frac…

Astrophysics of Galaxies (astro-ph.GA)Astrophysics::Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of GalaxiesAstrophysics::Galaxy Astrophysics
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