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Updated: Jun 5, 2025

Production of Membrane-Filtered Phase-Shift Decafluorobutane Nanodroplets from Preformed Microbubbles
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Finite Bubble Statistics Constrain Late Cosmological Phase Transitions.

Gilly Elor1, Ryusuke Jinno2,3, Soubhik Kumar4,5,6

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This study explores cosmic phase transitions, revealing how bubble nucleation fluctuations generate universal curvature fluctuations. These findings constrain dark-sector phase transitions, offering stronger limits than current neutrino measurements.

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Area of Science:

  • Cosmology
  • Particle Physics
  • Astrophysics

Background:

  • Late-time first-order cosmological phase transitions (PTs) occur below standard model temperatures.
  • Stochastic bubble nucleation in these PTs creates superhorizon fluctuations in completion time.

Purpose of the Study:

  • To compute how these fluctuations source universal curvature fluctuations.
  • To constrain the energy released in dark-sector PTs using observational data.

Main Methods:

  • Analyzing superhorizon fluctuations from stochastic bubble nucleation.
  • Utilizing cosmic microwave background (CMB) and large scale structure measurements for constraints.
  • Comparing derived constraints with existing bounds (e.g., ΔNeff) and future projections (e.g., CMB-S4).

Main Results:

  • Fluctuations in PT completion time universally source curvature fluctuations.
  • Constraints on dark-sector PT energy release are derived for temperatures 0.1 eV≲T_{PT}≲keV.
  • These constraints are more stringent than current ΔNeff bounds and some CMB-S4 projections.

Conclusions:

  • The study provides a novel method to probe early universe physics through gravitational effects.
  • Future CMB spectral distortions and pulsar timing arrays will offer competitive sensitivity for higher PT temperatures (keV≲T_{PT}≲GeV).