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Positive evidence for neutrino oscillations is mounting from the solar and atmospheric neutrino anomalies and the LSND experiment. Accordingly, the neutrino mass differences appear to lie in the sub-eV range and at least some of the mixing…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Raffelt

We explore scenarios where the highest energy cosmic rays are produced by new particle physics near the grand unification scale. Using detailed numerical simulations of extragalactic nucleon, gamma-ray, and neutrino propagation, we show the…

高能物理 - 唯象学 · 物理学 2009-10-31 Guenter Sigl , Sangjin Lee , Pijushpani Bhattacharjee , Shigeru Yoshida

The propagation of $\gamma$ rays over very large distances provides new insights on the intergalactic medium and on fundamental physics. On their path to the Earth, $\gamma$ rays can annihilate with diffuse infrared or optical photons of…

高能天体物理现象 · 物理学 2016-07-20 Dieter Horns , Agnieszka Jacholkowska

A long-standing problem in astrophysics is to measure the mass associated with galaxies. Gravitational lensing provides one of the cleanest ways to make this measurement. To date, the most powerful lensing probes of galactic mass have been…

天体物理学 · 物理学 2009-09-29 Scott Dodelson , Glenn D. Starkman

Many new physics scenarios contain ultralight scalars, states which are either exactly massless or much lighter than any other massive particle in the model. Axions and majorons constitute well-motivated examples of this type of particle.…

高能物理 - 唯象学 · 物理学 2021-04-14 Pablo Escribano , Avelino Vicente

Ultralight particles, with a mass below the electronvolt scale, exhibit wave-like behavior and have arisen as a compelling dark matter candidate. A particularly intriguing subclass is scalar dark matter, which induces variations in…

高能物理 - 唯象学 · 物理学 2026-02-10 Xucheng Gan , Da Liu , Di Liu , Xuheng Luo , Bingrong Yu

It has been confirmed experimentally the existence of a mass gap between Standard Model (SM) and eventual Beyond Standard Model (BSM) fields. Therefore, the use of effective approaches to search for fingerprints of New Physics is very…

高能物理 - 唯象学 · 物理学 2023-09-27 Ignasi Rosell , Antonio Pich , Juan Jose Sanz-Cillero

Ultra-light scalar fields may explain the nature of the dark matter in our universe. If such scalars couple quadratically to particles of the Standard Model the scalar acquires an effective mass which depends on the local matter energy…

高能物理 - 唯象学 · 物理学 2026-03-04 Clare Burrage , Angus Macdonald , Michael P. Ross , Gray Rybka , Elisa Todarello

Neutron star mergers, referring to both binary neutron star and neutron star black hole mergers, are the canonical multimessenger events. They have been detected across the electromagnetic spectrum, have recently been detected in…

We entertain the novel possibility that long range forces may lead to violations of accidental symmetries, in particular baryon number. Employing an ultralight scalar, with a mass $\ll$ eV, we illustrate that this scenario can lead to…

高能物理 - 唯象学 · 物理学 2023-08-02 Hooman Davoudiasl

Massive stars (>8 $M_{\odot}$) often undergo intense mass loss through winds or eruptive events in the final stages of their evolution, leading to the formation of a dense circumstellar medium (CSM). This material, expelled months to years…

高能天体物理现象 · 物理学 2025-10-15 Silvia Gagliardini , Simone Dall'Osso , Dafne Guetta , Angela Zegarelli , Silvia Celli , Antonio Capone , Irene Di Palma

Many instruments for astroparticle physics are primarily geared towards multi-messenger astrophysics, to study the origin of cosmic rays (CR) and to understand high-energy astrophysical processes. Since these instruments observe the…

高能天体物理现象 · 物理学 2024-03-01 Markus Ackermann , Klaus Helbing

Superluminous supernovae (SLSNe) are rare transients that are $\sim 10 - 100$ times more luminous than ordinary stellar explosions, reaching peak optical luminosities $\sim 10^{44} - 10^{45}$ erg s$^{-1}$. The energy source powering SLSNe…

高能天体物理现象 · 物理学 2026-03-27 Mainak Mukhopadhyay , Shigeo S. Kimura , Indrek Vurm , Brian D. Metzger

Ultralight scalars, which are states that are either exactly massless or much lighter than any other massive particle in the model, appear in many new physics scenarios. Axions and majorons constitute well-motivated examples of this type of…

高能物理 - 唯象学 · 物理学 2021-04-30 Pablo Escribano

Ultra-light scalar fields, with masses of between m=10^{-33} eV and m=10^{-22} eV, can affect the growth of structure in the Universe. We identify the different regimes in the evolution of ultra-light scalar fields, how they affect the…

高能物理 - 唯象学 · 物理学 2010-12-23 David J. E. Marsh , Pedro G. Ferreira

We construct families, and concrete examples, of simple extensions of the Standard Model that can yield ultralight {real or} complex vectors or scalars with potential astrophysical relevance. Specifically, the mass range for these putative…

Charged Higgs boson can exist in many physics beyond the standard models (BSM) and it is the obvious BSM signal. We briefly describe why the 125GeV scalar discovered at the LHC must have (heavy) companion: the charged Higgs boson, in a new…

高能物理 - 唯象学 · 物理学 2014-10-17 Shou-hua Zhu

The LHC experiments have searched for and excluded many proposed Beyond the Standard Model (BSM) theories. However, there are many scenarios where LHC has little or no sensitivity. Electron-positron colliders offers a different avenue for…

高能物理 - 唯象学 · 物理学 2022-12-13 Mikael Berggren

The situation in particle physics after the discovery of the Higgs boson is discussed. Is the Standard Model consistent quantum field theory? Does it describe all experimental data? Are there any indications of physics beyond the SM? Is…

高能物理 - 唯象学 · 物理学 2015-12-01 D. I. Kazakov

We propose that the ultralight dark matter (ULDM) model, in which dark matter particles have a tiny mass of $m=O(10^{-22})eV$, has characteristic scales for physical quantities of observed galaxies such as mass, size, acceleration, mass…

星系天体物理 · 物理学 2025-04-24 Jae-Weon Lee