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相关论文: Axino Mass in Supergravity Models

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In the framework where the strong coupling is dynamical, the QCD sector may confine at a much higher temperature than it would in the Standard Model, and the temperature-dependent mass of the QCD axion evolves in a non-trivial way. We find…

高能物理 - 唯象学 · 物理学 2022-01-12 Lucien Heurtier , Fei Huang , Tim M. P. Tait

It is shown that a supersymmetric SO(10) model extended with fermion singlets can accommodate the observed neutrino masses and mixings as well as generate the desired lepton asymmetry in concordance with the gravitino constraint. A…

高能物理 - 唯象学 · 物理学 2008-11-26 Swarup Kumar Majee , Mina K. Parida , Amitava Raychaudhuri

Motivated by specific connections to dark matter signatures, we study the prospects of observing the presence of a relatively light gluino whose mass is in the range ~(500-900) GeV with a wino-like lightest supersymmetric particle with mass…

高能物理 - 唯象学 · 物理学 2010-04-30 Daniel Feldman , Gordon Kane , Ran Lu , Brent D. Nelson

We explore the dark matter detection prospects in the Minimal Supersymmetric Standard Model in the scenario where the scalar partners of the fermions and the Higgs particles (except for the Standard-Model-like one) are assumed to be very…

高能物理 - 唯象学 · 物理学 2009-08-24 Nicolas Bernal

We discuss a new mechanism for baryogenesis, in which the baryon asymmetry is generated by the lightest particle in another sector, for example the supersymmetric particle (LSP), decaying to quarks via baryonic-number-violating…

高能物理 - 唯象学 · 物理学 2015-05-27 Angelo Monteux , Chang Sub Shin

We study a scenario allowing a solution of the strong charge parity problem via the Peccei-Quinn mechanism, implemented in gravity with torsion. In this framework there appears a torsion-related pseudoscalar field known as Kalb-Ramond…

高能物理 - 唯象学 · 物理学 2015-04-14 Oscar Castillo-Felisola , Cristobal Corral , Sergey Kovalenko , Ivan Schmidt , Valery E. Lyubovitskij

We study in detail a supersymmetric Peccei-Quinn model, which has a DFSZ and a KSVZ version. The fields breaking the Peccei-Quinn (PQ) symmetry correspond to flat directions (flaton fields) and have unsuppressed couplings when PQ symmetry…

高能物理 - 唯象学 · 物理学 2007-05-23 E. J. Chun , D. Comelli , David H. Lyth

We propose a novel framework that simultaneously addresses three critical issues: tiny neutrino masses and their mixing patterns, dark matter, and the strong CP problem. Our model extends the Peccei-Quinn (PQ) symmetry by incorporating…

高能物理 - 唯象学 · 物理学 2025-08-15 Sin Kyu Kang , Hiroshi Okada

Motivated by the flavored Peccei-Quinn symmetry for unifying the flavor physics and string theory, we construct an explicit model by introducing a $U(1)$ symmetry such that the $U(1)_X$-$[gravity]^2$ anomaly-free condition together with the…

高能物理 - 唯象学 · 物理学 2017-07-26 Y. H. Ahn

We present a minimal Grand Unified Theory model, based on $SU(5)$ gauge symmetry and a global $U(1)$ Peccei-Quinn symmetry, that predicts the existence of an ultralight axion dark matter within a narrow mass range of…

高能物理 - 唯象学 · 物理学 2023-08-02 Stefan Antusch , Ilja Doršner , Kevin Hinze , Shaikh Saad

The axion not only solves the strong CP puzzle, but it also may be the main constituent of cold dark matter. We review the axion dark matter predictions for the case that the Peccei-Quinn symmetry is restored after inflation.

高能物理 - 唯象学 · 物理学 2018-05-28 Andreas Ringwald

We study constraints on the models of bosonic super-weakly interacting particle (super-WIMP) dark matter (DM) with DM masses $m_X \sim \mathcal{O}(1 - 100)$ keV from leptonic decays $M\rightarrow \ell \bar{\nu}_\ell + X$, where $M=B^\pm,…

高能物理 - 唯象学 · 物理学 2015-06-03 Y. G. Aditya , Kristopher J. Healey , Alexey A. Petrov

I will talk on my recent works. Axino, related to the SUSY transformation of axion, can mix with Goldstino in principle. In this short talk, I would like to explain what is the axino mass and its plausible mass range. The axino mass is…

高能物理 - 唯象学 · 物理学 2012-11-05 Jihn E. Kim , Min-Seok Seo

The QCD axion is widely studied as a dark matter (DM) candidate and as a solution to the strong CP problem of the Standard Model. In conventional field-theoretic models, a much larger mass scale than the electroweak (EW) scale is typically…

高能物理 - 唯象学 · 物理学 2024-12-30 Wen Yin

In some supergravity models, the superlight gravitino is accompanied by a light weakly coupled scalar (S) and pseudo-scalar (P) particle. The coupling of these particles to matter is inversely proportional to the product of the gravitino…

高能物理 - 唯象学 · 物理学 2009-10-30 J. A. Grifols , R. N. Mohapatra , A. Riotto

We discuss the effective interactions of axion supermultiplet, which might be important for analyzing the cosmological aspect of supersymmetric axion model. Related to axino cosmology, it is stressed that three seemingly similar but…

高能物理 - 唯象学 · 物理学 2011-08-24 Kyu Jung Bae , Kiwoon Choi , Sang Hui Im

Axino and gravitino are promising candidates to solve the dark matter (DM) problem in the framework of supersymmetry. In this work, we assume that the axino is the lightest supersymmetric particle (LSP), and therefore contributes to DM. In…

高能物理 - 唯象学 · 物理学 2020-02-05 German A. Gomez-Vargas , Daniel E. Lopez-Fogliani , Carlos Munoz , Andres D. Perez

Among various supersymmetric (SUSY) models, gauge-mediated SUSY breaking models with an ultra-light gravitino of mass m_{3/2} \lesssim O(10) eV are very attractive, since they are completely free from notorious gravitino problems. A…

高能物理 - 唯象学 · 物理学 2008-11-26 K. Hamaguchi , S. Shirai , T. T. Yanagida

In recently introduced Split Susy theories, in which the scale of Susy breaking is very high, the requirement that the relic abundance of the Lightest SuperPartner (LSP) provides the Dark Matter of the Universe leads to the prediction of…

高能物理 - 唯象学 · 物理学 2009-11-10 Leonardo Senatore

We study the constraints on neutralino dark matter in minimal low energy supersymmetry models and the case of heavy lepton and quark scalar superpartners. For values of the Higgsino and gaugino mass parameters of the order of the weak…

高能物理 - 唯象学 · 物理学 2017-05-31 Peisi Huang , Roger A. Roglans , Daniel D. Spiegel , Yitian Sun , Carlos E. M. Wagner