Search results for "Inflation"

showing 10 items of 210 documents

Fiscal Adjustment and Business Cycle Synchronization

2013

Using a panel of annual data for 20 countries we show that synchronized fiscal consolidation (stimulus) programmes in different countries make their business cycles more closely linked, especially in the case of fiscal adjustments lasting 2 or 3 years. We also find: (i) little evidence of decoupling when an inflation targeting regime is unilaterally adopted; (ii) an increase in business cycle synchronization when countries fix their exchange rates and become members of a monetary union; (iii) a positive effect of bilateral trade on the synchronization of business cycles.

Bilateral tradeStimulus (economics)Consolidation (business)jel:C41Inflation targetingjel:E62EconomicsBusiness cycleMonetary economicsBusiness cycle synchronizationFiscal consolidation fiscal stimulus business cycle synchronizationSSRN Electronic Journal
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Norm-inflation results for purely BBM-type Boussinesq systems

2022

This article is concerned with the norm-inflation phenomena associated with a periodic initial-value abcd-Benjamin-Bona-Mahony type Boussinesq system. We show that the initial-value problem is ill-posed in the periodic Sobolev spaces H−sp (0, 2π)×H−sp (0, 2π) for all s > 0. Our proof is constructive, in the sense that we provide smooth initial data that generates solutions arbitrarily large in H−sp (0, 2π) × H−sp (0, 2π)-norm for arbitrarily short time. This result is sharp since in [15] the well-posedness is proved to holding for all positive periodic Sobolev indexes of the form Hsp (0, 2π) × Hsp (0, 2π), including s = 0. peerReviewed

Boussinesq systemnorm inflationPicard's iterationosittaisdifferentiaaliyhtälötBenjamin-Bona Mahony equationApplied MathematicsFourier'n sarjatDuhamel's principleFourier seriesspectral analysisAnalysisJournal of Mathematical Analysis and Applications
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Stochastic Episodes of Latent Cytomegalovirus Transcription Drive CD8 T-Cell “Memory Inflation” and Avoid Immune Evasion

2021

Acute infection with murine cytomegalovirus (mCMV) is controlled by CD8+ T cells and develops into a state of latent infection, referred to as latency, which is defined by lifelong maintenance of viral genomes but absence of infectious virus in latently infected cell types. Latency is associated with an increase in numbers of viral epitope-specific CD8+ T cells over time, a phenomenon known as “memory inflation” (MI). The “inflationary” subset of CD8+ T cells has been phenotyped as KLRG1+CD62L- effector-memory T cells (iTEM). It is agreed upon that proliferation of iTEM requires repeated episodes of antigen presentation, which implies that antigen-encoding viral genes must be transcribed du…

CD4-Positive T-LymphocytesGene Expression Regulation Viral0301 basic medicineMuromegaloviruslatent infectionTime FactorsTranscription Geneticeffector memory CD8+ T cellsAntigen presentationImmunologyBiologyVirusImmediate-Early Proteins03 medical and health sciences0302 clinical medicineImmune systemImmunityAnimalsCytotoxic T cellImmunology and AllergyLatency (engineering)Antigens ViralLungGenememory inflationlatencyOriginal Researchimmune evasionMice Inbred BALB CStochastic ProcessesModels ImmunologicalHerpesviridae InfectionsRC581-607VirologyVirus LatencyDisease Models Animalvirus reactivationantigen presentationPhenotype030104 developmental biologyHost-Pathogen Interactionsgene expressionFemaleVirus ActivationImmunologic diseases. AllergyImmunologic MemoryCD8030215 immunologyFrontiers in Immunology
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Primordial dark matter from curvature induced symmetry breaking

2020

We demonstrate that adiabatic dark matter can be generated by gravity induced symmetry breaking during inflation. We study a $Z_2$ symmetric scalar singlet that couples to other fields only through gravity and for which the symmetry is broken by the spacetime curvature during inflation when the non-minimal coupling $\xi$ is negative. We find that the symmetry breaking leads to the formation of adiabatic dark matter with the observed abundance for the singlet mass $m\sim{\rm MeV}$ and $|\xi|\sim 1$.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciences114 Physical sciencessymmetry breakingGeneral Relativity and Quantum Cosmologypimeä aineGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesprimordial dark matterSymmetry breakinginflationAdiabatic processMathematical physicsPhysicsInflation (cosmology)symmetriadark matter theory010308 nuclear & particles physicsAstronomy and AstrophysicsCoupling (probability)Symmetry (physics)quantum field theory on curved spaceHigh Energy Physics - PhenomenologyAstrophysics - Cosmology and Nongalactic Astrophysics
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CMB spectral distortions in generic two-field models

2017

We investigate the CMB $\mu$ distortion in models where two uncorrelated sources contribute to primordial perturbations. We parameterise each source by an amplitude, tilt, running and running of the running. We perform a detailed analysis of the distribution signal as function of the model parameters, highlighting the differences compared to single-source models. As a specific example, we also investigate the mixed inflaton-curvaton scenario. We find that the $\mu$ distortion could efficiently break degeneracies of curvaton parameters especially when combined with future sensitivity of probing the tensor-to-scalar ratio $r$. For example, assuming bounds $\mu < 0.5 \times 10^{-8}$ and $r<0.0…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)ART. NO. 023505Cosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesCosmologyHigh Energy Physics - Phenomenology (hep-ph)EARLY UNIVERSEDistortion0103 physical sciencesphysics of the early universeENERGY-RELEASEStatistical physicsSensitivity (control systems)inflation010303 astronomy & astrophysicsPhysicsInflation (cosmology)010308 nuclear & particles physicscosmological parameters from CMBRCURVATURE PERTURBATIONCONSTRAINTSAstronomy and AstrophysicsFunction (mathematics)115 Astronomy Space scienceMIXED INFLATONHigh Energy Physics - PhenomenologyDENSITY PERTURBATIONSAmplitudeCOSMOLOGYRADIATIONAstrophysics - Cosmology and Nongalactic AstrophysicsGENERATIONJournal of Cosmology and Astroparticle Physics
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Testing theories of Gravity and Supergravity with inflation and observations of the cosmic microwave background

2016

Many extensions of Einstein's theory of gravity have been studied and proposed with various motivations like the quest for a quantum theory of gravity to extensions of anomalies in observations at the solar system, galactic and cosmological scales. These extensions include adding higher powers of Ricci curvature $R$, coupling the Ricci curvature with scalar fields and generalized functions of $R$. In addition when viewed from the perspective of Supergravity (SUGRA) many of these theories may originate from the same SUGRA theory interpreted in different frames. SUGRA therefore serves as a good framework for organizing and generalizing theories of gravity beyond General Relativity. All these …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectFOS: Physical sciencesLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)CMBSUGRA01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyMetric expansion of spacesymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckinflation010306 general physicsMathematical Physicsmedia_commonPhysics010308 nuclear & particles physicsAstronomy and AstrophysicsUniverseHigh Energy Physics - PhenomenologySpace and Planetary SciencesymbolsDark energyCMB; inflation; SUGRAAstrophysics - Cosmology and Nongalactic Astrophysics
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Axion star nucleation in dark minihalos around primordial black holes

2020

We consider a general class of axion models, including the QCD and string axion, in which the PQ symmetry is broken before or during inflation. Assuming the axion is the dominant component of the dark matter, we discuss axion star formation in virialized dark minihalos around primordial black holes through gravitational Bose-Einstein condensation. We determine the conditions for minihalos to kinetically produce axion stars before galaxy formation. Today, we expect up to $\sim 10^{17}$ ($\sim 10^9$) axion stars in a radius of 100 parsecs around the Sun for the case of the QCD (string) axion.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsDark matterFOS: Physical sciencesmustat aukotPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicshiukkasfysiikka01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGalaxy formation and evolution010306 general physicsAxionAstrophysics::Galaxy AstrophysicsPhysicsInflation (cosmology)010308 nuclear & particles physicsStar formationHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyStarsydinfysiikkaAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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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
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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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Slow-roll corrections in multi-field inflation: a separate universes approach

2018

In view of cosmological parameters being measured to ever higher precision, theoretical predictions must also be computed to an equally high level of precision. In this work we investigate the impact on such predictions of relaxing some of the simplifying assumptions often used in these computations. In particular, we investigate the importance of slow-roll corrections in the computation of multi-field inflation observables, such as the amplitude of the scalar spectrum $P_\zeta$, its spectral tilt $n_s$, the tensor-to-scalar ratio $r$ and the non-Gaussianity parameter $f_{NL}$. To this end we use the separate universes approach and $\delta N$ formalism, which allows us to consider slow-roll…

DYNAMICSCosmology and Nongalactic Astrophysics (astro-ph.CO)ComputationFOS: Physical sciencesCMB01 natural sciences114 Physical sciences0103 physical sciencesStatistical physicsinflationMULTICOMPONENT INFLATON010303 astronomy & astrophysicsPhysicsSPECTRUMSlow roll010308 nuclear & particles physicsEquations of motionCONSTRAINTSAstronomy and AstrophysicsObservableCOSMOLOGICAL PERTURBATIONSEXPANSION115 Astronomy Space scienceAmplitudeHypersurfacecosmological perturbation theoryCompact formMulti field2ND-ORDERAPPROXIMATIONGENERATIONAstrophysics - Cosmology and Nongalactic Astrophysics
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