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Resonant decay of flat directions

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Resonant decay of flat directions. / Postma, Marieke; Mazumdar, Anupam.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2004, No. 1, 5, 20.01.2004.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Postma, M & Mazumdar, A 2004, 'Resonant decay of flat directions', Journal of Cosmology and Astroparticle Physics, vol. 2004, no. 1, 5. https://doi.org/10.1088/1475-7516/2004/01/005

APA

Postma, M., & Mazumdar, A. (2004). Resonant decay of flat directions. Journal of Cosmology and Astroparticle Physics, 2004(1), Article 5. https://doi.org/10.1088/1475-7516/2004/01/005

Vancouver

Postma M, Mazumdar A. Resonant decay of flat directions. Journal of Cosmology and Astroparticle Physics. 2004 Jan 20;2004(1):5. doi: 10.1088/1475-7516/2004/01/005

Author

Postma, Marieke ; Mazumdar, Anupam. / Resonant decay of flat directions. In: Journal of Cosmology and Astroparticle Physics. 2004 ; Vol. 2004, No. 1.

Bibtex

@article{486a4b3b13a441b089abca244e9f0aa1,
title = "Resonant decay of flat directions",
abstract = "We study preheating, i.e., non-perturbative resonant decay, of flat direction fields, concentrating on MSSM flat directions and the right handed sneutrino. The difference between inflaton preheating and flaton preheating, is that the potential is more constraint in the latter case. The effects of a complex driving field, quartic couplings in the potential, and the presence of a thermal bath are important and cannot be neglected. Preheating of MSSM flat directions is typically delayed due to out-of-phase oscillations of the real and imaginary components and may be preceded by perturbative decay or $Q$-ball formation. Particle production due to the violation of adiabaticity is expected to be inefficient due to back reaction effects. For a small initial sneutrino VEV, $ \lesssim m_N/h$ with $m_N$ the mass of the right handed sneutrino and $h$ a yakawa coupling, there are tachyonic instabilities. The $D$-term quartic couplings do not generate an effective mass for the tachyonic modes, making it an efficient decay channel. It is unclear how thermal scattering affects the resonance.",
keywords = "inflation, baryon asymmetry",
author = "Marieke Postma and Anupam Mazumdar",
note = "20 pages, 4 figures",
year = "2004",
month = jan,
day = "20",
doi = "10.1088/1475-7516/2004/01/005",
language = "English",
volume = "2004",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Resonant decay of flat directions

AU - Postma, Marieke

AU - Mazumdar, Anupam

N1 - 20 pages, 4 figures

PY - 2004/1/20

Y1 - 2004/1/20

N2 - We study preheating, i.e., non-perturbative resonant decay, of flat direction fields, concentrating on MSSM flat directions and the right handed sneutrino. The difference between inflaton preheating and flaton preheating, is that the potential is more constraint in the latter case. The effects of a complex driving field, quartic couplings in the potential, and the presence of a thermal bath are important and cannot be neglected. Preheating of MSSM flat directions is typically delayed due to out-of-phase oscillations of the real and imaginary components and may be preceded by perturbative decay or $Q$-ball formation. Particle production due to the violation of adiabaticity is expected to be inefficient due to back reaction effects. For a small initial sneutrino VEV, $ \lesssim m_N/h$ with $m_N$ the mass of the right handed sneutrino and $h$ a yakawa coupling, there are tachyonic instabilities. The $D$-term quartic couplings do not generate an effective mass for the tachyonic modes, making it an efficient decay channel. It is unclear how thermal scattering affects the resonance.

AB - We study preheating, i.e., non-perturbative resonant decay, of flat direction fields, concentrating on MSSM flat directions and the right handed sneutrino. The difference between inflaton preheating and flaton preheating, is that the potential is more constraint in the latter case. The effects of a complex driving field, quartic couplings in the potential, and the presence of a thermal bath are important and cannot be neglected. Preheating of MSSM flat directions is typically delayed due to out-of-phase oscillations of the real and imaginary components and may be preceded by perturbative decay or $Q$-ball formation. Particle production due to the violation of adiabaticity is expected to be inefficient due to back reaction effects. For a small initial sneutrino VEV, $ \lesssim m_N/h$ with $m_N$ the mass of the right handed sneutrino and $h$ a yakawa coupling, there are tachyonic instabilities. The $D$-term quartic couplings do not generate an effective mass for the tachyonic modes, making it an efficient decay channel. It is unclear how thermal scattering affects the resonance.

KW - inflation

KW - baryon asymmetry

U2 - 10.1088/1475-7516/2004/01/005

DO - 10.1088/1475-7516/2004/01/005

M3 - Journal article

VL - 2004

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 1

M1 - 5

ER -