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We investigate the production of dark matter with non-standard momentum distributions arising from the decay of a relativistic massive neutrino into a lighter fermion and boson H$\rightarrow$F$+$B. We develop the Boltzmann equations for…

天体物理学 · 物理学 2009-10-22 G. D. Starkman , N. Kaiser , R. A. Malaney

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

Neutron stars are excellent emitters of gravitational waves. Squeezing matter beyond nuclear densities invites exotic physical processes, many of which violently transfer large amounts of mass at relativistic velocities, disrupting…

高能天体物理现象 · 物理学 2015-11-20 Paul D. Lasky

The spectrum of frequencies and characteristic times that compose the ringdown phase of gravitational waves emitted by neutron stars carries information about the matter content (the equation of state) and the underlying theory of gravity.…

广义相对论与量子宇宙学 · 物理学 2020-07-01 Jose Luis Blázquez-Salcedo , Fech Scen Khoo , Jutta Kunz

Ultralight bosons around comparable-mass binaries can form gravitationally bound states analogous to molecules once the binary separation decreases below the boson's Bohr radius, with the inner region co-moving with the binary. We simulate…

广义相对论与量子宇宙学 · 物理学 2025-09-15 Yuhao Guo , Zhen Zhong , Yifan Chen , Vitor Cardoso , Taishi Ikeda , Lihang Zhou

A single magnetic fluxon moving at a high velocity in a Josephson multilayer (e.g., high-temperature superconductor such as BSCCO) can emit electromagnetic waves (Cherenkov radiation), which leads to formation of novel stable dynamic states…

超导电性 · 物理学 2009-10-31 E. Goldobin , B. A. Malomed , A. V. Ustinov

Superradiant instability of ultralight bosons can produce clouds around rotating black holes, whose continuous gravitational wave (GW) emission is a promising observational target. Precise predictions of the signal frequency and its…

广义相对论与量子宇宙学 · 物理学 2026-04-24 Takuya Takahashi

Numerous investigations discuss neutrino properties from low to ultra high energies. This review discusses several topics that are investigated in present day experiments. The first section covers the detection of $\tau$-neutrinos of cosmic…

高能物理 - 唯象学 · 物理学 2017-08-18 E. A. Paschos

We calculate the flux of neutrinos generated by the propagation of ultra-high energy iron over cosmological distances and show that even if ultra-high energy cosmic rays are composed of heavy nuclei, a significant flux of high-energy…

天体物理学 · 物理学 2008-11-26 Maximo Ave , N. Busca , A. V. Olinto , A. A. Watson , T. Yamamoto

We investigate the scattered field from $N$ identical two-level atoms resonantly driven by a weak coherent field in a one-dimensional waveguide. For atoms separated by the drive wavelength, increasing the number of atoms progressively…

量子物理 · 物理学 2025-06-06 Zeidan Zeidan , Therese Karmstrand , Maryam Khanahmadi , Göran Johansson

Nonlinear Thomson and Compton processes, in which energetic electrons collide with an intense optical pulse, are investigated in the framework of classical and quantum electrodynamics. Spectral modulations of the emitted radiation,…

高能物理 - 唯象学 · 物理学 2015-06-17 K. Krajewska , M. Twardy , J. Z. Kamiński

Cosmogenic neutrinos originate from interactions of cosmic rays propagating through the universe with cosmic background photons. Since both high-energy cosmic rays and cosmic background photons exist, the existence of high-energy cosmogenic…

高能天体物理现象 · 物理学 2019-06-19 David Wittkowski , Karl-Heinz Kampert

Gigantic neutrino telescopes are primarily designed to search for very high energy neutrino radiation from the cosmos. Neutrinos travel unhindered over cosmological distances and therefore carry unique undistorted information about its…

高能天体物理现象 · 物理学 2012-06-13 M. Ribordy

If high-energy neutrinos propagate in a background of ultralight scalar field particles of dark matter ($m_\varphi \sim 10^{-23}$eV), neutrino-dark matter interactions can play a role and affect the neutrino flux. In this work we analyse…

高能物理 - 唯象学 · 物理学 2016-06-01 Matías M. Reynoso , Oscar A. Sampayo

Tentative evidence suggests that the cores of massive neutron stars consist of deconfined quark matter. We argue that the formation of such a quark matter core during a galactic supernova could be accompanied by the emission of…

高能物理 - 唯象学 · 物理学 2026-03-20 Katarina Bleau , Joachim Kopp , Jiheon Lee , Jorinde van de Vis

As the technology of gravitational-wave and neutrino detectors becomes increasingly mature, a multi-messenger era of astronomy is ushered in. Advanced gravitational wave detectors are close to making a ground-breaking discovery of…

高能天体物理现象 · 物理学 2015-06-16 He Gao , Bing Zhang , Xue-Feng Wu , Zi-Gao Dai

Recently, a new theory based on superluminal tunnelling has been proposed to explain the transition of highly energetic neutrinos propagating in matter to tachyonic states. In this work, we determine the possible mechanisms that lead…

综合物理 · 物理学 2020-02-07 Luca Nanni

Black hole superradiance is a powerful tool in the search for ultra-light bosons. Constraints on the existence of such particles have been derived from the observation of highly spinning black holes, absence of continuous gravitational-wave…

高能物理 - 唯象学 · 物理学 2021-11-19 Andrea Caputo , Samuel J. Witte , Diego Blas , Paolo Pani

Ultralight bosons are a class of hypothetical particles that could potentially solve critical problems in fields ranging from cosmology to astrophysics and fundamental physics. If ultralight bosons exist, they form clouds around spinning…

广义相对论与量子宇宙学 · 物理学 2022-09-13 Kelvin H. M. Chan , Otto A. Hannuksela

Ultrahigh energy neutrinos can be used to explore the physics at the TeV scale. We study the neutrino-nucleon cross section in models with extra dimensions and the fundamental scale at the TeV. In particular, we discuss the production of…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Masip