Search results for "Background Radiation"

showing 10 items of 55 documents

In the realm of the Hubble tension—a review of solutions

2021

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with en…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)satellite: PlanckPhysics and Astronomy (miscellaneous)gravitation: modelPhysics beyond the Standard ModelCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsbaryon: oscillation: acoustic01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)cosmological model: parameter space0103 physical sciencesstructurePlanckinflationcosmic background radiation: power spectrum010306 general physicsdark energyneutrino: interactionPhysicssupernova: Type IHubble constant010308 nuclear & particles physicsnew physicsmagnetic field: primordialtensionredshiftAstrophysics - Astrophysics of GalaxiesRedshiftrecombinationHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]relativisticsymbolsDark energy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Phenomenology (particle physics)statisticalAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Chronic Background Radiation Correlates With Sperm Swimming Endurance in Bank Voles From Chernobyl

2022

Sperm quantity and quality are key features explaining intra- and interspecific variation in male reproductive success. Spermatogenesis is sensitive to ionizing radiation and laboratory studies investigating acute effects of ionizing radiation have indeed found negative effects of radiation on sperm quantity and quality. In nature, levels of natural background radiation vary dramatically, and chronic effects of low-level background radiation exposure on spermatogenesis are poorly understood. The Chernobyl region offers a unique research opportunity for investigating effects of chronic low-level ionizing radiation on reproductive properties of wild organisms. We captured male bank voles (Myo…

Ecologymetsämyyräionisoiva säteilytaustasäteilylisääntyminensperm morphometrysäteilybiologiareproductionbackground radiationsiittiötMyodes glareolusEcology Evolution Behavior and Systematicsperformancefysiologiset vaikutukset
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Environmental Gamma Radiation Measurements on the Island of Pantelleria

1992

The population exposure to those living on the island of Pantelleria, Italy, was estimated by measuring the natural gamma background. Gamma spectra of natural rocks and measurements of absorbed dose in air were taken. A correlation was found between the mean gamma exposure rate and the mean values of natural radionuclide concentrations in the investigated rocks.

Geological PhenomenaRadionuclideeducation.field_of_studyEpidemiologyHealth Toxicology and MutagenesisPopulationRadiochemistryGeologyRadiationAtmospheric sciencesDisastersMediterranean IslandsItalyGamma RaysRadiation MonitoringAbsorbed doseRadioactive contaminationBackground RadiationEnvironmental scienceDosimetryRadiology Nuclear Medicine and imagingPopulation exposureeducationNatural radioactivityEnvironmental MonitoringHealth Physics
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Robustness of cosmological axion mass limits

2015

We present cosmological bounds on the thermal axion mass in an extended cosmological scenario in which the primordial power spectrum of scalar perturbations differs from the usual power-law shape predicted by the simplest inflationary models. The power spectrum is instead modeled by means of a "piecewise cubic Hermite interpolating polynomial" (PCHIP). When using Cosmic Microwave Background measurements combined with other cosmological data sets, the thermal axion mass constraints are degraded only slightly. The addition of the measurements of $\sigma_8$ and $\Omega_m$ from the 2013 Planck cluster catalogue on galaxy number counts relaxes the bounds on the thermal axion mass, mildly favouri…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundScalar (mathematics)Cosmic background radiationFOS: Physical sciencesFísicaSpectral densityAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesake13. Climate action0103 physical sciencessymbolsPlanckNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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Interacting dark energy in a closed universe

2020

Recent measurements of the Cosmic Microwave Anisotropies power spectra measured by the Planck satellite show a preference for a closed universe at more than $99 \%$ Confidence Level. Such a scenario is however in disagreement with several low redshift observables, including luminosity distances of Type Ia Supernovae. Here we show that Interacting Dark Energy (IDE) models can ease the discrepancies between Planck and Supernovae Ia data in a closed Universe. Therefore IDE cosmologies remain as very appealing scenarios, as they can provide the solution to a number of observational tensions in different fiducial cosmologies. The results presented here strongly favour broader analyses of cosmolo…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic background radiationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyLuminositysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Vacuum energy0103 physical sciencesPlanckFlatness (cosmology)010303 astronomy & astrophysicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsUniverseRedshiftHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Space and Planetary SciencesymbolsDark energyAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society: Letters
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Revising the Predictions of Inflation for the Cosmic Microwave Background Anisotropies

2009

4 pages, 1 figure.-- PACS nrs.: 98.70.Vc; 11.10.Gh; 98.80.Cq.-- ArXiv pre-print available at: http://arxiv.org/abs/0901.0439

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)[PACS] Cosmic background radiations01 natural sciencesGeneral Relativity and Quantum CosmologySpectral lineRenormalizationHigh Energy Physics - Phenomenology (hep-ph)[PACS] Particle-theory and field-theory models of the early UniverseQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsSpectral densityCMB cold spot3. Good healthHigh Energy Physics - Phenomenology[PACS] Renormalization in quantum field theoryHigh Energy Physics - Theory (hep-th)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Impact of general reionization scenarios on extraction of inflationary parameters

2010

Determination of whether the Harrison-Zel'dovich spectrum for primordial scalar perturbations is consistent with observations is sensitive to assumptions about the reionization scenario. In light of this result, we revisit constraints on inflationary models using more general reionization scenarios. While the bounds on the tensor-to-scalar ratio are largely unmodified, when different reionization schemes are addressed, hybrid models are back into the inflationary game. In the general reionization picture, we reconstruct both the shape and amplitude of the inflaton potential. We discuss how relaxing the simple reionization restriction affects the reconstruction of the potential through the c…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonCMB cold spotCosmologyGeneral Relativity and Quantum CosmologyFísica nuclearReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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Fitness costs of increased cataract frequency and cumulative radiation dose in natural mammalian populations from Chernobyl

2015

AbstractA cataract is a clouding of the lens that reduces light transmission to the retina and it decreases the visual acuity of the bearer. The prevalence of cataracts in natural populations of mammals and their potential ecological significance, is poorly known. Cataracts have been reported to arise from high levels of oxidative stress and a major cause of oxidative stress is ionizing radiation. We investigated whether elevated frequencies of cataracts are found in eyes of bank voles Myodes glareolus collected from natural populations in areas with varying levels of background radiation in Chernobyl. We found high frequencies of cataracts in voles collected from different areas in Chernob…

Male0301 basic medicineVisual acuitygenetic structuresOffspringtaustasäteilyPhysiology010501 environmental sciencesRadiation DosageChernobyl Nuclear Accidentmedicine.disease_cause01 natural sciencesArticleIonizing radiationChernobylToxicology03 medical and health sciencesbackground radiationCataractskaihiRadiation IonizingMyodes glareolusmedicineAnimalsbank voleRadiation Injuries0105 earth and related environmental sciencesMammalsMultidisciplinarybiologyArvicolinaeRadiation dosemedicine.diseasebiology.organism_classificationeye diseasesfitness costs030104 developmental biologyChernobyl Nuclear AccidentArvicolinaecataractta1181Femalesense organsmedicine.symptomradiation doseOxidative stressScientific Reports
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Dark radiation and interacting scenarios

2013

An extra dark radiation component can be present in the universe in the form of sterile neutrinos, axions or other very light degrees of freedom which may interact with the dark matter sector. We derive here the cosmological constraints on the dark radiation abundance, on its effective velocity and on its viscosity parameter from current data in dark radiation-dark matter coupled models. The cosmological bounds on the number of extra dark radiation species do not change significantly when considering interacting schemes. We also find that the constraints on the dark radiation effective velocity are degraded by an order of magnitude while the errors on the viscosity parameter are a factor of…

Nuclear and High Energy PhysicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterCosmological parametersCosmic background radiationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyRadiacióPower spectrumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsAxionTelescopeDigital sky surveyPhysicsCosmologiaHubble constant010308 nuclear & particles physicsSpectral densityMicrowave background anisotropiesHigh Energy Physics - Phenomenology13. Climate actionDark radiationConstraintssymbolsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Updated CMB and x- and gamma-ray constraints on Majoron dark matter

2013

The Majoron provides an attractive dark matter candidate, directly associated with the mechanism responsible for spontaneous neutrino mass generation within the standard model SU(3)(c) circle times SU(2)(L) circle times U(1)(Y) framework. Here we update the cosmological and astrophysical constraints on Majoron dark matter coming from the cosmic microwave background and a variety of x- and gamma-ray observations.

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsAstrophysics::High Energy Astrophysical PhenomenaXMM-newton observationsDark matterCosmic microwave backgroundCosmic background radiationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesStandard ModelObservational cosmology0103 physical sciences010306 general physicsMajoronPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFísica13. Climate actionSterile neutrinosNeutrino
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