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Related papers: The TeV-mass curvaton

200 papers

Numerous observations point towards the existence of an unknown elementary particle with no electromagnetic interactions, a large population of which was presumably produced in the early stages of the history of the Universe. This so-called…

High Energy Physics - Phenomenology · Physics 2015-06-16 Alejandro Ibarra , David Tran , Christoph Weniger

A baryonic bound state with a mass of O(100) TeV, which is composed of strongly interacting messenger quarks in the low scale gauge mediation, can naturally be the cold dark matter. Interestingly, we find that such a baryonic dark matter is…

High Energy Physics - Phenomenology · Physics 2010-01-15 Koichi Hamaguchi , Eita Nakamura , Satoshi Shirai , T. T. Yanagida

Thermal dark matter that couples more strongly to electrons and photons than to neutrinos will heat the electron-photon plasma relative to the neutrino background if it becomes nonrelativistic after the neutrinos decouple from the thermal…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Chiu Man Ho , Robert J. Scherrer

We build a realistic model of curvaton cosmology, in which the energy content is described by radiation, WIMP dark matter and a curvaton component. We calculate the curvature and isocurvature perturbations, allowing for arbitrary initial…

Astrophysics · Physics 2008-11-26 Martin Lemoine , Jerome Martin

Utilizing the Fermi measurement of the gamma-ray spectrum toward the Galactic Center, we derive some of the strongest constraints to date on the dark matter (DM) lifetime in the mass range from hundreds of MeV to above an EeV. Our…

High Energy Physics - Phenomenology · Physics 2019-06-24 Timothy Cohen , Kohta Murase , Nicholas L. Rodd , Benjamin R. Safdi , Yotam Soreq

Recently, a number of authors have challenged the conventional assumption that the string scale, Planck mass, and unification scale are roughly comparable. It has been suggested that the string scale could be as low as a TeV. In this note,…

High Energy Physics - Theory · Physics 2010-02-03 Tom Banks , Ann Nelson , Michael Dine

We study three astrophysical/cosmological consequences of nonminimal couplings to gravity in wavelike vector dark matter. In the nonrelativistic limit, the nonminimal coupling with the lowest mass dimension leads to effective…

Cosmology and Nongalactic Astrophysics · Physics 2023-08-02 Hong-Yi Zhang , Siyang Ling

We consider the possibility that supersymmetry is broken above the inflationary mass scale and that the only "low" energy remnant of supersymmetry is the gravitino with mass of order the EeV scale. The gravitino in this class of models…

High Energy Physics - Phenomenology · Physics 2017-08-09 Emilian Dudas , Yann Mambrini , Keith Olive

Dark matter with mass in the crossover range between wave dark matter and particle dark matter, around $(10^{-3},\, 10^3)\,$eV, remains relatively unexplored by terrestrial experiments. In this mass regime, dark matter scatters coherently…

High Energy Physics - Phenomenology · Physics 2026-03-31 Pengshun Luo , Shigeki Matsumoto , Jie Sheng , Chuan-Yang Xing , Lin Zhu , Zhi-Jie Zhuge

We present a complete analysis of the cosmological constraints on decaying dark matter. Previous analyses have used the cosmic microwave background and Type Ia supernova. We have updated them with the latest data as well as extended the…

High Energy Physics - Phenomenology · Physics 2014-11-18 Santiago De Lope Amigo , William Man-Yin Cheung , Zhiqi Huang , Siew-Phang Ng

We argue that the curvaton decay takes place most naturally by way of a broad parametric resonance. The mechanism is analogous to resonant inflaton decay but does not require any tuning of the curvaton coupling strength to other scalar…

Astrophysics · Physics 2014-11-18 K. Enqvist , S. Nurmi , G. I. Rigopoulos

Among the several strategies for indirect searches of dark matter, one very promising one is to look for the gamma-rays from decaying dark matter. Here we use the most up-to-date upper bounds on the gamma-ray flux from $10^5$ to $10^{11}$…

High Energy Physics - Phenomenology · Physics 2021-11-17 Marco Chianese , Damiano F. G. Fiorillo , Rasmi Hajjar , Gennaro Miele , Ninetta Saviano

We study a model where two scalar fields, that are subdominant during inflation, decay into radiation some time after inflation has ended but before primordial nucleosynthesis. Perturbations of these two curvaton fields can be responsible…

High Energy Physics - Phenomenology · Physics 2008-11-26 Hooshyar Assadullahi , Jussi Valiviita , David Wands

Recently there has been a lot of interest in models in which gravity becomes strong at the TeV scale. The observed weakness of gravitational interactions is then explained by the existence of extra compact dimensions of space, which are…

High Energy Physics - Phenomenology · Physics 2009-10-31 Schuyler Cullen , Maxim Perelstein

We present the cosmological constraints on the cross section of baryon-dark matter interactions for the dark matter mass below the MeV scale from the Planck CMB (cosmic microwave background) and SDSS (Sloan Digital Sky Survey)…

Cosmology and Nongalactic Astrophysics · Physics 2019-09-25 Junpei Ooba , Horoyuki Tashiro , Kenji Kadota

The standard model weak interactions can be described by four-fermion V-A operators at low energies. New physics at the TeV scale can, however, generate the other Lorentz structures. In this talk, we review the constraints on such…

High Energy Physics - Lattice · Physics 2012-04-02 Tanmoy Bhattacharya , Rajan Gupta , Anosh Joseph , Huey-Wen Lin , Saul D. Cohen

We describe an approach to detect dark matter and other invisible particles with mass below a GeV, exploiting missing energy-momentum measurements and other kinematic features of fixed-target production. In the case of an invisibly decaying…

High Energy Physics - Phenomenology · Physics 2015-05-27 Eder Izaguirre , Gordan Krnjaic , Philip Schuster , Natalia Toro

We derive lower bounds for the Higgs-curvature coupling from vacuum stability during inflation in three inflationary models: quadratic and quartic chaotic inflation, and Starobinsky-like power-law inflation. In contrast to most previous…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-24 Andreas Mantziris , Tommi Markkanen , Arttu Rajantie

We study Compton scattering, gamma e -> gamma e, in the context of the recent proposal for Weak Scale Quantum Gravity (WSQG) with large extra dimensions. It is shown that, with an ultraviolet cutoff $M_S \sim 1$ TeV for the effective…

High Energy Physics - Phenomenology · Physics 2016-09-06 Hooman Davoudiasl