Results 291 to 300 of about 896,961 (328)
Thermal gravitons from warm inflation
In warm inflation (WI), the persistent thermal bath that is sustained by dissipative interactions with the inflaton field produces a stochastic background of gravitational waves (GWs).
Gabriele Montefalcone +3 more
semanticscholar +3 more sources
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Warm Inflation with the Standard Model.
Physical Review LettersWe show for the first time that warm inflation is feasible with standard model (SM) gauge interactions alone. Our model consists of a minimal extension of the SM by a single scalar inflaton field with an axionlike coupling to gluons and a monomial ...
K. V. Berghaus +2 more
semanticscholar +1 more source
WI2easy: warm inflation dynamics made easy
Journal of Cosmology and Astroparticle PhysicsWe present WI2easy, a Mathematica package for high-precision analysis of warm inflation (WI) dynamics, enabling efficient computation of both background evolution and curvature perturbations.
Gabriel S. Rodrigues, Rudnei O. Ramos
semanticscholar +1 more source
Viability of warm inflation with standard model interactions
Physical Review DThe minimal warm inflation scenario proposed in Ref. [1] -- featuring an axionlike inflaton coupled to Standard Model (SM) gluons via the standard interaction $\phi G \tilde G$ -- offers a compelling bridge between inflationary dynamics and SM particle ...
Rudnei O. Ramos, Gabriel S. Rodrigues
semanticscholar +1 more source
Purely gravitational dark matter production in warm inflation
Physical Review DWe consider an appealing scenario for the production of purely gravitational dark matter in the background of warm inflation, a mechanism that maintains stable thermal bath during inflation.
Qing-Yang Wang +3 more
semanticscholar +1 more source
Unraveling the Hubble tension with warm inflation
Classical and quantum gravityThe validity of warm inflation is investigated in the light of recent CMB missions in both strong and weak dissipative regimes. The tensor to scalar ratio of various inflationary models is found to be consistent with the recent CMB results for different ...
Anupama B, P. K. Suresh
semanticscholar +1 more source
The α-attractor E-Model in warm inflation: observational viability from Planck 2018
Journal of Cosmology and Astroparticle PhysicsWe explore the inflationary evolution and observational viability of the α-attractor E-model in the framework of warm inflation, focusing on both weak and strong dissipative regimes, with a dissipation coefficient linear in temperature.
Bhargabi Saha, M. Nandy
semanticscholar +1 more source
Warm Inflation in $f(Q)$ gravity
Chinese Physics C, High Energy Physics & Nuclear PhysicsWe investigate warm inflation in the framework of $f(Q)$ gravity within a Friedmann-Robertson-Walker spacetime. Unlike cold inflation, where the inflaton evolves in isolation, warm inflation features continuous interaction between the inflaton field ...
Tuhina Ghorui +3 more
semanticscholar +1 more source
Dark Matter Production during Warm Inflation via Freeze-In.
Physical Review LettersWe present a novel perspective on the role of inflation in the production of dark matter (DM). Specifically, we explore the DM production during warm inflation via ultraviolet freeze-in (WIFI).
Katherine Freese +2 more
semanticscholar +1 more source
Stage IV CMB forecasts for warm inflation
Journal of Cosmology and Astroparticle PhysicsWe report forecast constraints on warm inflation in the light of future cosmic microwave background (CMB) surveys, with data expected to be available in the coming decade.
F. dos Santos +3 more
semanticscholar +1 more source

