Standard

Near-inflection point inflation and production of dark matter during reheating. / Ghoshal, Anish; Lambiase, Gaetano; Pal, Supratik и др.

2022. Работа представлена на Bled Workshops in Physics.

Результаты исследований: Материалы конференций › материалы › Рецензирование

Harvard

Ghoshal, A, Lambiase, G, Pal, S, Paul, A & Порей, Ш 2022, 'Near-inflection point inflation and production of dark matter during reheating', Работа представлена на Bled Workshops in Physics, 01.01.2022.

APA

Ghoshal, A., Lambiase, G., Pal, S., Paul, A., & Порей, Ш. (2022). Near-inflection point inflation and production of dark matter during reheating. Работа представлена на Bled Workshops in Physics.

Vancouver

Ghoshal A, Lambiase G, Pal S, Paul A, Порей Ш. Near-inflection point inflation and production of dark matter during reheating. 2022. Работа представлена на Bled Workshops in Physics.

Author

Ghoshal, Anish ; Lambiase, Gaetano ; Pal, Supratik и др. / Near-inflection point inflation and production of dark matter during reheating. Работа представлена на Bled Workshops in Physics.18 стр.

BibTeX

@conference{c14cbc97ad6a4b8c8a59a2e9e6ca2ea2,
title = "Near-inflection point inflation and production of dark matter during reheating",
abstract = "We study slow roll single eld in ationary scenario and the production of non thermal fermionic dark matter, together with standard model Higgs, during reheating. For the in ationary scenario, we have considered two models of polynomial potential one is symmetric about the origin and another one is not. We x the coe cients of the potential from the current Cosmic Microwave Background (CMB) data from Planck/Bicep. Next, we explore the allowed parameter space on the coupling (y ) with in aton and mass (m) of dark matter (DM) particles ( ) produced during reheating and satisfying CMB and several other cosmological constraints",
author = "Anish Ghoshal and Gaetano Lambiase and Supratik Pal and Arnab Paul and Шиладитья Порей",
note = " Shiladitya Porey wants to thank Professor Norma Susana Mankoc Borstnik, Professor Maxim Khlopov, Professor Astri Kleppe, and the organizers of the Bled 25th Workshop. Work of Shiladitya Porey is funded by RSF Grant 19-42-02004. Supratik Pal thanks Department of Science and Technology, Govt. of India for partial support through Grant No. NMICPS/006/MD/2020-21; Bled Workshops in Physics ; Conference date: 01-01-2022",
year = "2022",
language = "English",

}

RIS

TY - CONF

T1 - Near-inflection point inflation and production of dark matter during reheating

AU - Ghoshal, Anish

AU - Lambiase, Gaetano

AU - Pal, Supratik

AU - Paul, Arnab

AU - Порей, Шиладитья

N1 - Shiladitya Porey wants to thank Professor Norma Susana Mankoc Borstnik, Professor Maxim Khlopov, Professor Astri Kleppe, and the organizers of the Bled 25th Workshop. Work of Shiladitya Porey is funded by RSF Grant 19-42-02004. Supratik Pal thanks Department of Science and Technology, Govt. of India for partial support through Grant No. NMICPS/006/MD/2020-21

PY - 2022

Y1 - 2022

N2 - We study slow roll single eld in ationary scenario and the production of non thermal fermionic dark matter, together with standard model Higgs, during reheating. For the in ationary scenario, we have considered two models of polynomial potential one is symmetric about the origin and another one is not. We x the coe cients of the potential from the current Cosmic Microwave Background (CMB) data from Planck/Bicep. Next, we explore the allowed parameter space on the coupling (y ) with in aton and mass (m) of dark matter (DM) particles ( ) produced during reheating and satisfying CMB and several other cosmological constraints

AB - We study slow roll single eld in ationary scenario and the production of non thermal fermionic dark matter, together with standard model Higgs, during reheating. For the in ationary scenario, we have considered two models of polynomial potential one is symmetric about the origin and another one is not. We x the coe cients of the potential from the current Cosmic Microwave Background (CMB) data from Planck/Bicep. Next, we explore the allowed parameter space on the coupling (y ) with in aton and mass (m) of dark matter (DM) particles ( ) produced during reheating and satisfying CMB and several other cosmological constraints

UR - https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85202355042&origin=inward

UR - https://arxiv.org/pdf/2211.15061

M3 - Paper

T2 - Bled Workshops in Physics

Y2 - 1 January 2022

ER -

ID: 68453807