中文
相关论文

相关论文: Revisiting Supernova 1987A Constraints on Dark Pho…

200 篇论文

Dark matter particles may bind with nuclei if there exists an attractive force of sufficient strength. We show that a dark photon mediator of mass $\sim (10 - 100)$ MeV that kinetically mixes with Standard Model electromagnetism at the…

高能物理 - 唯象学 · 物理学 2021-10-14 Asher Berlin , Hongwan Liu , Maxim Pospelov , Harikrishnan Ramani

The recently observed very high energy (VHE) photons dubbed as GRB221009A by several terrestrial observatories such as LHAASO and Carpet-2 require a physics explanation beyond the standard model. Such energetic gamma ray bursts, originating…

高能物理 - 唯象学 · 物理学 2024-09-27 M. Afif Ismail , Chrisna Setyo Nugroho , Qidir Maulana Binu Soesanto

If large extra dimensions exist in nature, supernova (SN) cores will emit large fluxes of Kaluza-Klein gravitons, producing a cosmic background of these particles with energies and masses up to about 100 MeV. Radiative decays then give rise…

高能物理 - 唯象学 · 物理学 2011-05-05 Steen Hannestad , Georg Raffelt

Numerous estimates of upper bounds on the (anti)neutrino rest mass have been published based on the SN1987A observations. Here, we use a nonkinematic (thermal) time extent to provide a rest mass estimate of a few eV (as mc^2 mass), if not…

综合物理 · 物理学 2009-10-05 John Michael Williams

Supernova 1987A offers a unique opportunity to study an evolving supernova in unprecedented detail over several decades. The X-ray emission is dominated by interactions between the ejecta and the circumstellar medium, primarily the…

高能天体物理现象 · 物理学 2021-08-11 Dennis Alp , Josefin Larsson , Claes Fransson

Since the dawn of the new millennium, there has been a revived interest in the concept of extra dimensions.In this scenario all the standard model matter and gauge fields are confined to the 4 dimensions and only gravity can escape to…

高能物理 - 唯象学 · 物理学 2011-04-11 V. H. Satheesh Kumar , P. K. Suresh , P. K. Das

We estimate the sensitivity of various experiments detecting ultra-high-energy cosmic rays to primary photons with energies above 10^19 eV. We demonstrate that the energy of a primary photon may be significantly (up to a factor of ~ 10)…

天体物理学 · 物理学 2009-11-19 O. E. Kalashev , G. I. Rubtsov , S. V. Troitsky

Distant supernovae have been observed to be fainter than what is expected in a matter dominated universe. The most likely explanation is that the universe is dominated by an energy component with negative pressure -- dark energy. However,…

天体物理学 · 物理学 2009-11-10 Linda Ostman , Edvard Mortsell

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…

高能物理 - 唯象学 · 物理学 2009-10-31 Schuyler Cullen , Maxim Perelstein

Dark photons are particles invoked in some extensions of the Standard Model which could account for at least part of the dark matter content of the Universe. It has been proposed that the production of dark photons in stellar interiors…

太阳与恒星天体物理 · 物理学 2020-01-08 Adrián Ayala , Ilidio Lopes , Antonio García Hernández , Juan Carlos Suárez , Íñigo Muñoz Elorza

We calculate the rate of production of hypothetical light vector bosons (LVBs) from nucleon-nucleon bremsstrahlung reactions in the soft radiation limit directly in terms of the measured nucleon-nucleon elastic cross sections. We use these…

核理论 · 物理学 2016-11-23 Ermal Rrapaj , Sanjay Reddy

We present the supernova constraints on an axion-photon-dark photon coupling, which can be the leading coupling to dark sector models and can also lead to dramatic changes to axion cosmology. We show that the supernova bound on this…

高能物理 - 唯象学 · 物理学 2021-07-14 Anson Hook , Gustavo Marques-Tavares , Clayton Ristow

If massless leptonic photons associated to electron, muon or tau leptonic number exist they would have been emitted from supernova 1987a via the annihilation process $\nu\bar{\nu}\to\gamma_{l}\gamma_{l}$. By requiring that this process does…

高能物理 - 唯象学 · 物理学 2009-10-30 S. N. Gninenko

We explore the cosmological consequences of kinetically mixed dark photons with a mass between 1 MeV and 10 GeV, and an effective electromagnetic fine structure constant as small as $10^{-38}$. We calculate the freeze-in abundance of these…

高能物理 - 唯象学 · 物理学 2014-09-05 Anthony Fradette , Maxim Pospelov , Josef Pradler , Adam Ritz

We derive a bound on dark photon dark matter scenarios where the dark photon mass is generated through the Higgs mechanism, based on the requirement that symmetry breaking must occur sufficiently early in the universe. We emphasize that…

高能物理 - 唯象学 · 物理学 2025-02-06 Naoya Kitajima , Shota Nakagawa , Fuminobu Takahashi , Wen Yin

I summarize the results of a recent analysis where the cosmological effects of interactions of neutrinos with cold Dark Matter (DM) is investigated. This interaction produces diffusion-damped oscillations in the matter power spectrum,…

天体物理学 · 物理学 2008-11-26 Gianpiero Mangano

The neutrino signal from SN~1987A provides an excellent opportunity to constrain physical theories for matter at extreme conditions and properties of particles that are produced in supernova (SN) cores. Phase transitions in the supranuclear…

天体物理学 · 物理学 2007-05-23 H. -Thomas Janka

We point out a new and largely model-independent constraint on the dark matter scattering cross section with nucleons, applying when this quantity is larger than for typical weakly interacting dark matter candidates. When the dark matter…

天体物理学 · 物理学 2008-11-26 Gregory D. Mack , John F. Beacom , Gianfranco Bertone

Using recent supernova models, I revisit the Supernova 1987a constraints on scalar/pseudoscalar Axion-Like-Particles (ALPs). On the basis of the neutrino detections, the luminosity of ALPs must be $\lesssim 5\times10^{52} \,\mathrm{erg}/s$…

高能物理 - 唯象学 · 物理学 2018-08-31 Jun Seok Lee

Majoron-like bosons would emerge from a supernova (SN) core by neutrino coalescence of the form $\nu\nu\to\phi$ and $\bar\nu\bar\nu\to\phi$ with 100 MeV-range energies. Subsequent decays to (anti)neutrinos of all flavors provide a flux…

高能物理 - 唯象学 · 物理学 2023-07-18 Damiano F. G. Fiorillo , Georg G. Raffelt , Edoardo Vitagliano