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Title: Supersymmetric Sneutrino-Higgs inflation

Abstract

It is shown that in the phenomenologically realistic supersymmetric MSSM theory, a linear combination of the neutral, up Higgs field with the third family left- and right-handed sneutrinos can play the role of the cosmological inflaton. Assuming that supersymmetry is softly broken at a mass scale of order , the potential energy associated with this field allows for 60 e-foldings of inflation with the cosmological parameters being consistent with all Planck2015 data. The theory does not require any non-standard coupling to gravity and the physical fields are all sub-Planckian during the inflationary epoch. It will be shown that there is a “robust” set of initial conditions which, in addition to satisfying the Planck data, simultaneously are consistent with all present LHC phenomenological requirements.

Authors:
; ;
Publication Date:
Research Org.:
Univ. of Pennsylvania, Philadelphia, PA (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
1328257
Alternate Identifier(s):
OSTI ID: 1425908
Grant/Contract Number:  
SC0007901
Resource Type:
Published Article
Journal Name:
Physics Letters B
Additional Journal Information:
Journal Name: Physics Letters B Journal Volume: 762 Journal Issue: C; Journal ID: ISSN 0370-2693
Publisher:
Elsevier
Country of Publication:
Netherlands
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS

Citation Formats

Deen, Rehan, Ovrut, Burt A., and Purves, Austin. Supersymmetric Sneutrino-Higgs inflation. Netherlands: N. p., 2016. Web. https://doi.org/10.1016/j.physletb.2016.09.059.
Deen, Rehan, Ovrut, Burt A., & Purves, Austin. Supersymmetric Sneutrino-Higgs inflation. Netherlands. https://doi.org/10.1016/j.physletb.2016.09.059
Deen, Rehan, Ovrut, Burt A., and Purves, Austin. Tue . "Supersymmetric Sneutrino-Higgs inflation". Netherlands. https://doi.org/10.1016/j.physletb.2016.09.059.
@article{osti_1328257,
title = {Supersymmetric Sneutrino-Higgs inflation},
author = {Deen, Rehan and Ovrut, Burt A. and Purves, Austin},
abstractNote = {It is shown that in the phenomenologically realistic supersymmetric MSSM theory, a linear combination of the neutral, up Higgs field with the third family left- and right-handed sneutrinos can play the role of the cosmological inflaton. Assuming that supersymmetry is softly broken at a mass scale of order , the potential energy associated with this field allows for 60 e-foldings of inflation with the cosmological parameters being consistent with all Planck2015 data. The theory does not require any non-standard coupling to gravity and the physical fields are all sub-Planckian during the inflationary epoch. It will be shown that there is a “robust” set of initial conditions which, in addition to satisfying the Planck data, simultaneously are consistent with all present LHC phenomenological requirements.},
doi = {10.1016/j.physletb.2016.09.059},
journal = {Physics Letters B},
number = C,
volume = 762,
place = {Netherlands},
year = {2016},
month = {11}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1016/j.physletb.2016.09.059

Citation Metrics:
Cited by: 2 works
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Works referencing / citing this record:

The R-parity violating decays of charginos and neutralinos in the B-L MSSM
journal, February 2019

  • Dumitru, Sebastian; Ovrut, Burt A.; Purves, Austin
  • Journal of High Energy Physics, Vol. 2019, Issue 2
  • DOI: 10.1007/jhep02(2019)124

The R-parity violating decays of charginos and neutralinos in the B-L MSSM
journal, February 2019

  • Dumitru, Sebastian; Ovrut, Burt A.; Purves, Austin
  • Journal of High Energy Physics, Vol. 2019, Issue 2
  • DOI: 10.1007/jhep02(2019)124

Perturbative reheating in Sneutrino-Higgs cosmology
journal, September 2018

  • Cai, Yong; Deen, Rehan; Ovrut, Burt A.
  • Journal of High Energy Physics, Vol. 2018, Issue 9
  • DOI: 10.1007/jhep09(2018)001

Non-vanishing heterotic superpotentials on elliptic fibrations
journal, September 2018

  • Buchbinder, Evgeny I.; Lin, Ling; Ovrut, Burt A.
  • Journal of High Energy Physics, Vol. 2018, Issue 9
  • DOI: 10.1007/jhep09(2018)111