Home > Research > Publications & Outputs > Baryogenesis, dark matter and inflation in the ...

Electronic data

  • art%3A10.1007%2FJHEP01%282014%29073

    Rights statement: JHEP is an open-access journal funded by SCOAP3 and licensed under CC BY 4.0 The original publication is available at www.link.springer.com

    Final published version, 796 KB, PDF document

Links

Text available via DOI:

View graph of relations

Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model. / Balazs, Csaba; Mazumdar, Anupam; Pukartas, Ernestas et al.
In: Journal of High Energy Physics, Vol. 2014, 73, 2014.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

APA

Balazs, C., Mazumdar, A., Pukartas, E., & White, G. (2014). Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model. Journal of High Energy Physics, 2014, Article 73. https://doi.org/10.1007/JHEP01(2014)073

Vancouver

Balazs C, Mazumdar A, Pukartas E, White G. Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model. Journal of High Energy Physics. 2014;2014:73. Epub 2014 Jan 16. doi: 10.1007/JHEP01(2014)073

Author

Balazs, Csaba ; Mazumdar, Anupam ; Pukartas, Ernestas et al. / Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model. In: Journal of High Energy Physics. 2014 ; Vol. 2014.

Bibtex

@article{6fd1e4119a734a3dac809421a2b812ae,
title = "Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model",
abstract = "Explaining baryon asymmetry, dark matter and inflation are important elements of a successful theory that extends beyond the Standard Model of particle physics. In this paper we explore these issues within the Next-to-Minimal Supersymmetric Standard Model (NMSSM), by studying the conditions for a strongly first order electroweak phase transition, the abundance of the lightest supersymmetric particle (LSP), and inflation driven by a gauge invariant flat direction of MSSM made up of right handed squarks. We present the regions of parameter space which can yield successful predictions for cosmic microwave background (CMB) radiation, the observed relic density for the neutralino LSP, and successful baryogenesis constrained by collider measurements, such as the recent Higgs mass bound, branching ratios of rare, flavour violating decays, and the invisible Z decay width. We also explore where dark matter interactions with xenon nuclei would fall within current bounds of XENON100 and the projected limits for the XENON1T and LUX experiments.",
keywords = "Supersymmetry, Baryogenesis, Dark matter, Inflation",
author = "Csaba Balazs and Anupam Mazumdar and Ernestas Pukartas and Graham White",
note = "JHEP is an open-access journal funded by SCOAP3 and licensed under CC BY 4.0 The original publication is available at www.link.springer.com",
year = "2014",
doi = "10.1007/JHEP01(2014)073",
language = "English",
volume = "2014",
journal = "Journal of High Energy Physics",
issn = "1029-8479",
publisher = "Springer-Verlag",

}

RIS

TY - JOUR

T1 - Baryogenesis, dark matter and inflation in the next-to-minimal supersymmetric standard model

AU - Balazs, Csaba

AU - Mazumdar, Anupam

AU - Pukartas, Ernestas

AU - White, Graham

N1 - JHEP is an open-access journal funded by SCOAP3 and licensed under CC BY 4.0 The original publication is available at www.link.springer.com

PY - 2014

Y1 - 2014

N2 - Explaining baryon asymmetry, dark matter and inflation are important elements of a successful theory that extends beyond the Standard Model of particle physics. In this paper we explore these issues within the Next-to-Minimal Supersymmetric Standard Model (NMSSM), by studying the conditions for a strongly first order electroweak phase transition, the abundance of the lightest supersymmetric particle (LSP), and inflation driven by a gauge invariant flat direction of MSSM made up of right handed squarks. We present the regions of parameter space which can yield successful predictions for cosmic microwave background (CMB) radiation, the observed relic density for the neutralino LSP, and successful baryogenesis constrained by collider measurements, such as the recent Higgs mass bound, branching ratios of rare, flavour violating decays, and the invisible Z decay width. We also explore where dark matter interactions with xenon nuclei would fall within current bounds of XENON100 and the projected limits for the XENON1T and LUX experiments.

AB - Explaining baryon asymmetry, dark matter and inflation are important elements of a successful theory that extends beyond the Standard Model of particle physics. In this paper we explore these issues within the Next-to-Minimal Supersymmetric Standard Model (NMSSM), by studying the conditions for a strongly first order electroweak phase transition, the abundance of the lightest supersymmetric particle (LSP), and inflation driven by a gauge invariant flat direction of MSSM made up of right handed squarks. We present the regions of parameter space which can yield successful predictions for cosmic microwave background (CMB) radiation, the observed relic density for the neutralino LSP, and successful baryogenesis constrained by collider measurements, such as the recent Higgs mass bound, branching ratios of rare, flavour violating decays, and the invisible Z decay width. We also explore where dark matter interactions with xenon nuclei would fall within current bounds of XENON100 and the projected limits for the XENON1T and LUX experiments.

KW - Supersymmetry

KW - Baryogenesis

KW - Dark matter

KW - Inflation

U2 - 10.1007/JHEP01(2014)073

DO - 10.1007/JHEP01(2014)073

M3 - Journal article

VL - 2014

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

SN - 1029-8479

M1 - 73

ER -