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New BBN limits on Physics Beyond the Standard Model from He4

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

A recent analysis of the He4 abundance determined from observations of extragalactic HII regions indicates a significantly greater uncertainty for the He4 mass fraction. The derived value is now in line with predictions from big bang nucleosynthesis when the baryon density determined by WMAP is assumed. Based on this new analysis of He4, we derive constraints on a host of particle properties which include: limits on the number of relativistic species at the time of BBN (commonly taken to be the limit on neutrino flavors), limits on the variations of fundamental couplings such as alpha_{em} and G_N, and limits on decaying particles.

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years

2026 1 2021 1

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representative citing papers

Superhorizon curvature perturbations in hybrid inflation revisited

astro-ph.CO · 2026-06-29 · conditional · novelty 6.0

Hybrid inflation's waterfall tachyonic instability grows isocurvature modes that convert to curvature perturbations at the field-space turn, yielding a k^{3}-peaked spectrum with always-positive f_NL that enhances PBH formation.

Scalar induced gravitational waves review

gr-qc · 2021-09-03 · unverdicted · novelty 2.0

A review that unifies analytical expressions for scalar-induced gravitational waves and emphasizes calculations for non-radiation-dominated cosmologies.

citing papers explorer

Showing 2 of 2 citing papers.

  • Superhorizon curvature perturbations in hybrid inflation revisited astro-ph.CO · 2026-06-29 · conditional · none · ref 152 · internal anchor

    Hybrid inflation's waterfall tachyonic instability grows isocurvature modes that convert to curvature perturbations at the field-space turn, yielding a k^{3}-peaked spectrum with always-positive f_NL that enhances PBH formation.

  • Scalar induced gravitational waves review gr-qc · 2021-09-03 · unverdicted · none · ref 300 · internal anchor

    A review that unifies analytical expressions for scalar-induced gravitational waves and emphasizes calculations for non-radiation-dominated cosmologies.