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Thermal pressure on ultrarelativistic bubbles from a semiclassical formalism

Long, Andrew J.; Turner, Jessica

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Authors

Andrew J. Long



Abstract

We study a planar bubble wall that is traveling at an ultrarelativistic speed through a thermal plasma. This situation may arise during a first-order electroweak phase transition in the early universe. As particles cross the wall, it is assumed that their mass grows from m a to m b , and they are decelerated causing them to emit massless radiation (m c = 0). We are interested in the momentum transfer to the wall, the thermal pressure felt by the wall, and the resultant terminal velocity of the wall. We employ the semiclassical current radiation (SCR) formalism to perform these calculations. An incident-charged particle is treated as a point-like classical electromagnetic current, and the spectrum of quantum electromagnetic radiation (photons) is derived by calculating appropriate matrix elements. To understand how the spectrum depends on the thickness of the wall, we explore simplified models for the current corresponding to an abrupt and a gradual deceleration. For the model of abrupt deceleration, we find that the SCR formalism can reproduce the P therm ∝ γ 0 w scaling found in earlier work by assuming that the emission is soft, but if the emission is not soft the SCR formalism can be used to obtain P therm ∝ γ 2 w instead. For the model of gradual deceleration, we find that the wall thickness L w enters to cutoff the otherwise log-flat radiation spectrum above a momentum of ∼ γ 2 w / L w , and we discuss the connections with classical electromagnetic bremsstrahlung.

Citation

Long, A. J., & Turner, J. (2024). Thermal pressure on ultrarelativistic bubbles from a semiclassical formalism. Journal of Cosmology and Astroparticle Physics, 2024(11), https://doi.org/10.1088/1475-7516/2024/11/024

Journal Article Type Article
Acceptance Date Oct 24, 2024
Online Publication Date Nov 19, 2024
Publication Date Nov 1, 2024
Deposit Date Nov 25, 2024
Publicly Available Date Nov 25, 2024
Journal Journal of Cosmology and Astroparticle Physics
Electronic ISSN 1475-7516
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 2024
Issue 11
DOI https://doi.org/10.1088/1475-7516/2024/11/024
Keywords cosmological phase transitions, physics of the early universe, primordial gravitational waves (theory)
Public URL https://durham-repository.worktribe.com/output/3104907

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