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相关论文: Heavy Light Inflaton and Dark Matter Production

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We consider a fermionic dark matter candidate interacting via a scalar mediator coupled with the Standard Model through a Higgs portal. We consider general setting including both scalar and pseudoscalar interactions between the scalar and…

高能物理 - 唯象学 · 物理学 2017-04-12 Kimmo Kainulainen , Kimmo Tuominen , Ville Vaskonen

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

高能物理 - 唯象学 · 物理学 2025-02-14 Antonio Torres Manso , Joao G. Rosa

Inflation can occur near a point of inflection in the potential of flat directions of the Minimal Supersymmetric Standard Model. In this paper we elaborate on the complementarity between the bounds from Cosmic Microwave Background…

高能物理 - 唯象学 · 物理学 2014-11-20 Rouzbeh Allahverdi , Bhaskar Dutta , Yudi Santoso

A generic prediction of the Coleman-Weinberg inflation is the existence of a heavy particle sector whose interactions with the inflaton, the lightest state in this sector, generate the inflaton potential at loop level. For typical…

高能物理 - 唯象学 · 物理学 2017-03-20 Kristjan Kannike , Antonio Racioppi , Martti Raidal

In this talk we will discuss how inflation can be embedded within a minimal extension of the Standard Model where the inflaton carries the Standard Model charges. There is no need of an ad-hoc scalar field to be introduced in order to…

高能物理 - 唯象学 · 物理学 2015-05-13 A. Mazumdar

We consider the Higgs portal $Z_2$ scalar model as the minimal extension of the Standard Model (SM) to incorporate the dark matter. We find that the dark matter mass is bounded to be lighter than 1000\,GeV within the framework that we have…

高能物理 - 唯象学 · 物理学 2015-06-19 Yuta Hamada , Hikaru Kawai , Kin-ya Oda

We suggest a minimal model for GeV-scale Majorana Dark Matter (DM) coupled to the standard model lepton sector via a charged scalar singlet. We show that there is an anti-correlation between the spin-independent DM-Nucleus scattering…

高能物理 - 唯象学 · 物理学 2021-04-21 Adil Jueid , Salah Nasri , Rachik Soualah

We investigate the production of a spectator scalar dark matter field that is directly coupled to the inflaton during inflation and reheating. We consider two specific inflationary potentials, namely the Starobinsky and T-model of…

高能物理 - 唯象学 · 物理学 2023-06-16 Marcos A. G. Garcia , Mathias Pierre , Sarunas Verner

We show that a minimal scenario, utilizing only the graviton as an intermediate messenger between the inflaton, the dark sector and the Standard Model (SM), is able to generate $simultaneously$ the observed relic density of dark matter…

高能物理 - 唯象学 · 物理学 2023-01-04 Basabendu Barman , Simon Cléry , Raymond T. Co , Yann Mambrini , Keith A. Olive

We study in detail a scenario in which the inflaton scalar field couples to both a visible sector (VS) and a hidden sector (HS). The VS is assumed to contain the Standard Model (SM), while the HS contains a dark matter (DM) candidate. We…

高能物理 - 唯象学 · 物理学 2026-05-12 Simon Cléry , Jean Kimus , Michel H. G. Tytgat

Building on recently constructed inflationary vector dark matter production mechanisms as well as studies of magnetogenesis, we show that an inflationary dark Schwinger mechanism can generate the observed dark matter relic abundance for…

高能物理 - 唯象学 · 物理学 2024-09-04 Mar Bastero-Gil , Paulo B. Ferraz , Lorenzo Ubaldi , Roberto Vega-Morales

A minimal candidate for dark matter is provided by a stable standard model singlet hermitian scalar field. The quantum mechanical effects of this singlet are explored in a model where the standard model Higgs boson has a large non-minimal…

高能物理 - 唯象学 · 物理学 2009-09-30 S. T. Love

There is strong evidence from cosmological data that the universe underwent an epoch of superluminal expansion called inflation. A satisfactory embedding of inflation in fundamental physics has been an outstanding problem at the interface…

高能物理 - 唯象学 · 物理学 2008-12-26 Rouzbeh Allahverdi

We propose a minimal model that can explain the electroweak scale, neutrino masses, Dark Matter (DM), and successful inflation all at once based on the multicritical-point principle (MPP). The model has two singlet scalar fields that…

高能物理 - 唯象学 · 物理学 2022-01-06 Yuta Hamada , Hikaru Kawai , Kiyoharu Kawana , Kin-ya Oda , Kei Yagyu

The initial density of dark matter (DM) particles, otherwise secluded from the standard model (SM), may be generated at reheating, with an initial temperature ratio for internal thermalizations, $\xi_i=T_{\rm DM,i}/T_{\rm SM,i}$. This…

高能物理 - 唯象学 · 物理学 2024-05-02 Deep Ghosh , Sourav Gope , Satyanarayan Mukhopadhyay

We argue that all the necessary ingredients for successful inflation are present in the flat directions of the Minimally Supersymmetric Standard Model. We show that out of many gauge invariant combinations of squarks, sleptons and Higgses,…

高能物理 - 唯象学 · 物理学 2008-11-26 Rouzbeh Allahverdi , Juan Garcia-Bellido , Kari Enqvist , Anupam Mazumdar

We present a scenario of vector dark matter production during inflation containing a complex inflaton field which is charged under a dark gauge field and which has a symmetry breaking potential. As the inflaton field rolls towards the…

高能物理 - 唯象学 · 物理学 2021-06-30 Hassan Firouzjahi , Mohammad Ali Gorji , Shinji Mukohyama , Borna Salehian

We study phenomenology of a light scalar dark matter (DM). In the model, there are an inert doublet scalar and a singlet Dirac fermion $\psi$, both charged under a global $Z_2$ symmetry. The mass of the lightest inert scalar $H$ can be…

高能物理 - 唯象学 · 物理学 2023-10-23 Ryo Higuchi , Syuhei Iguro , Shohei Okawa , Yuji Omura

The primordial inflation dilutes all matter except the quantum fluctuations which we see in the cosmic microwave background (CMB) radiation. Therefore the last phases of inflation must be embedded within a beyond the Standard Model (SM)…

高能物理 - 唯象学 · 物理学 2013-02-06 Celine Boehm , Jonathan Da Silva , Anupam Mazumdar , Ernestas Pukartas

We study models of inflation where the inflaton corresponds to a flat direction in field space and its mass term is generated by gravity mediated soft supersymmetry breaking at high scale. Assuming the inflaton to have non negligible…

高能物理 - 唯象学 · 物理学 2007-05-23 Laura Covi