Pith. sign in

REVIEW 3 cited by

Resonant decay of Bose condensates

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv hep-ph/9610477 v3 pith:GHB63ZOT submitted 1996-10-24 hep-ph

classification hep-ph
keywords bosedecayfluctuationsresultsanalyticalanotherapproximationcalculations
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

We present results of fully non-linear calculations of decay of the inflaton interacting with another scalar field X. Combining numerical results for cosmologically interesting range of resonance parameter, q \leq 10^6, with analytical estimates, we extrapolate them to larger q. We find that scattering of X fluctuations off the Bose condensate is a very efficient mechanism limiting growth of X fluctuations. For a single-component X, the resulting variance, at large q, is much smaller than that obtained in the Hartree approximation.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Particle decay as asymptotic narrow parametric resonance

    hep-ph 2025-05 conditional novelty 6.0 of 10

    A Boltzmann equation with Gaussian momentum spread reproduces the asymptotic growth rate and number density of narrow parametric resonance to within about 20 percent.

  2. Ephemeral Oscillons in Scalar-Tensor Theories: The Higgs-like case

    hep-ph 2025-01 conditional novelty 6.0 of 10

    In a Higgs-like Einstein-Cartan inflation model, oscillons formed after inflation are short-lived and their decay drives radiation domination within about four e-folds.

  3. Equation of state during (p)reheating with trilinear interactions

    astro-ph.CO 2025-07 unverdicted novelty 5.0 of 10

    Lattice simulations show that the post-inflationary equation of state with trilinear interactions returns to zero after an initial deviation, substantially lowering stochastic gravitational wave amplitudes relative to...

Pith tools