0000000000345006

AUTHOR

Tomo Takahashi

showing 2 related works from this author

The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe

2020

It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later. While the abundance of light elements indicates that the Universe was radiation dominated during Big Bang Nucleosynthesis (BBN), there is scant evidence that the Universe was radiation dominated prior to BBN. It is therefore possible that the cosmological history was more complicated, with deviations from the standard radiation domination during the earliest epochs. Indeed, several interesting proposals regarding various topics such as the generation of dark matter, matter-antimatter asymmetry, gravitational waves,…

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)reheatingmedia_common.quotation_subjectnucleosynthesis: big bangDark matterFOS: Physical sciencesPrimordial black holeGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologydark matterGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesenergy: density010306 general physicsmedia_commonInflation (cosmology)Physics010308 nuclear & particles physicsGravitational wave[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]gravitational radiationAstronomyUniverseinflation: modelBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]history[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]black hole: primordialasymmetryAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

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
researchProduct