Search results for "p-p"

showing 10 items of 3659 documents

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 lepton asymmetry with a nonzero mixing angle \theta13

2012

While the baryon asymmetry of the Universe is nowadays well measured by cosmological observations, the bounds on the lepton asymmetry in the form of neutrinos are still significantly weaker. We place limits on the relic neutrino asymmetries using some of the latest cosmological data, taking into account the effect of flavor oscillations. We present our results for two different values of the neutrino mixing angle \theta_{13}, and show that for large \theta_{13} the limits on the total neutrino asymmetry become more stringent, diluting even large initial flavor asymmetries. In particular, we find that the present bounds are still dominated by the limits coming from Big Bang Nucleosynthesis, …

Astrophysics and AstronomyNuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectCosmic microwave backgroundCosmic background radiationAstrophysics::Cosmology and Extragalactic AstrophysicsEarly Universe7. Clean energy01 natural sciencesAsymmetryPartícules (Física nuclear)CosmologyBaryon asymmetryBig Bang nucleosynthesisPower Spectrum0103 physical sciences010306 general physicsTelescopemedia_commonPhysicsFlavor Oscillations010308 nuclear & particles physicsHigh Energy Physics::Phenomenology[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]ConstraintsParametersNeutrino DegeneracyHigh Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsLepton
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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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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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Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons

2017

High energy cosmic ray electrons plus positrons (CREs), which lose energy quickly during their propagation, provide an ideal probe of Galactic high-energy processes and may enable the observation of phenomena such as dark-matter particle annihilation or decay. The CRE spectrum has been directly measured up to $\sim 2$ TeV in previous balloon- or space-borne experiments, and indirectly up to $\sim 5$ TeV by ground-based Cherenkov $\gamma$-ray telescope arrays. Evidence for a spectral break in the TeV energy range has been provided by indirect measurements of H.E.S.S., although the results were qualified by sizeable systematic uncertainties. Here we report a direct measurement of CREs in the …

Astrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayElectron01 natural sciencesdark matterHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Positroncosmic rays0103 physical sciences010303 astronomy & astrophysicsCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic rays dark matter electrons space experimentsMultidisciplinaryAnnihilation010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleSpectrum (functional analysis)electronsGalaxyHigh Energy Physics - PhenomenologyHigh Energy Physics::Experimentspace experimentsAstrophysics - High Energy Astrophysical Phenomena
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Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data

2013

Aims. We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Methods. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. Results. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to …

Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeMonte Carlo methodgamma-ray burst: generalFOS: Physical sciencesddc:500.201 natural sciencesCoincidenceSpectral lineGamma ray burstsmethods: numericalNuclear physicsneutrinoHigh Energy Physics - Phenomenology (hep-ph)Raigs gamma0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutrinsNeutrinos010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics:Desenvolupament humà i sostenible [Àrees temàtiques de la UPC]Muonnumerical [Methods]010308 nuclear & particles physicsneutrinosAstronomy and Astrophysicsgeneral [Gamma-ray burst]neutrinos - gamma-ray burst: general - methods: numerical; methods: numerical; neutrinos; gamma-ray burst: generalHigh Energy Physics - PhenomenologyGamma-ray burst: general; Methods: numerical; NeutrinosNeutrino detectorSpace and Planetary ScienceFISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoneutrinos - gamma-ray burst: general - methods: numericalGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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