English
Related papers

Related papers: The puzzling MILAGRO hot spots

200 papers

In this review paper, we present the main aspects of high-energy cosmic neutrino astrophysics. We begin by describing the generic expectations for cosmic neutrinos, including the effects of propagation from their sources to the detectors.…

High Energy Astrophysical Phenomena · Physics 2020-09-07 Andrea Palladino , Maurizio Spurio , Francesco Vissani

The BATSE experiment has now observed more than 1100 gamma-ray bursts. The observed angular distribution is isotropic, while the brightness distribution of bursts shows a reduced number of faint events. These observations favor a…

Astrophysics · Physics 2009-10-28 Dieter Hartmann , Ramesh Narayan

Current galaxy formation models predict the existence of X-ray-emitting gaseous halos around Milky Way (MW)-type galaxies. To investigate properties of this coronal gas in MW-like galaxies, we analyze a suite of high-resolution simulations…

We develop a first-principles formalism to compute the distortion to the relic neutrino density field caused by the peculiar motions of large-scale structures. This distortion slows halos down due to dynamical friction, causes a local…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-14 Caio Nascimento , Marilena Loverde

This is a review of high energy neutrino astronomy that might be done with a kilometer-scale detector. The emphasis is on diffuse neutrinos of extragalactic origin and their relation to possible sources of the highest energy cosmic rays,…

Astrophysics · Physics 2007-05-23 T. K. Gaisser

We propose a new hypothesis for the origin of non-solar hadronic cosmic rays (CRs) at all energies: Highly relativistic, narrowly collimated jets from the birth or collapse of neutron stars (NSs) in our Galaxy accelerate ambient disk and…

Astrophysics · Physics 2007-05-23 R. Plaga , O. C. de Jager , A. Dar

Secondary photons from decays of metastable neutralinos can contribute to the ultra-high energy cosmic ray flux. The neutralino production rate is too low in acceleration mechanisms to affect the cosmic ray spectrum without emitting…

Astrophysics · Physics 2007-05-23 D. S. Gorbunov , S. V. Troitsky

We discuss the difference between the distribution of secondaries measured in terms of pseudorapidity and that using the correct rapidity variable. We show a set of examples obtained using Monte Carlo simulations. We also consider the…

High Energy Physics - Phenomenology · Physics 2010-10-12 V. A. Schegelsky , M. G. Ryskin , A. D. Martin , V. A. Khoze

The possibility that the observed Ultra High Energy Cosmic Rays are generated by high energy neutrinos creating "Z-bursts" in resonant interactions with the background neutrinos has been proposed, but there are difficulties in generating…

High Energy Physics - Phenomenology · Physics 2007-05-23 B. H. J. Mckellar , M. Garbutt , G. J. Stephenson , T. Goldman

The sources of ultrahigh-energy cosmic rays (UHECRs) have been difficult to catch. It was recently pointed out that while sources of UHECR protons exhibit anisotropy patterns that become denser and compressed with rising energy,…

The Type-II Seesaw Model provides an attractive scenario to account for Majorana-neutrino masses. Its extended Higgs sector, if sufficiently light, can have a rich and distinctive phenomenology at the LHC while yielding automatically an…

High Energy Physics - Phenomenology · Physics 2024-10-30 Otilia A. Ducu , Ana E. Dumitriu , Adam Jinaru , Romain Kukla , Emmanuel Monnier , Gilbert Moultaka , Alexandra Tudorache , Hanlin Xu

A new type of gravitational microlensing experiment toward a field where stars are not resolved is being developed observationally and theoretically: pixel lensing. When the experiment is carried out toward the M31 bulge area, events may be…

Astrophysics · Physics 2009-10-28 Cheongho Han , Andrew Gould

The intense magnetic fields of neutron stars naturally lead to strong anisotropy and polarization of radiation emanating from their surfaces, both being sensitive to the hot spot position on the surface. Accordingly, pulse phase-resolved…

High Energy Astrophysical Phenomena · Physics 2025-02-21 Matthew G. Baring , Hoa Dinh Thi , George A. Younes , Kun Hu

Within the "pseudo-Dirac" scenario for massive neutrinos the existence of sterile neutrinos which are almost degenerate in mass with the active ones is hypothesized. The presence of these sterile neutrinos can affect the flavor composition…

High Energy Physics - Phenomenology · Physics 2010-02-11 Arman Esmaili

Light antinuclei, like antideuteron and antihelium-3, are ideal probes for new, exotic physics because their astrophysical backgrounds are suppressed at low energies. In order to exploit fully the inherent discovery potential of light…

High Energy Physics - Phenomenology · Physics 2023-03-22 M. Kachelriess , S. Ostapchenko , J. Tjemsland

We consider the possibility that Dirac neutrino masses may be a manifestation of chiral symmetry breaking via non-perturbative QCD dynamics. The key role played by light quarks in this mechanism can naturally lead to signals that are…

High Energy Physics - Phenomenology · Physics 2022-05-19 Hooman Davoudiasl , Ian M. Lewis , Matthew Sullivan

I show that it may be possible to explain the present evidence for a gamma-ray emission from the galactic halo as due to halo WIMP annihilations. Not only the intensity and spatial pattern of the halo emission can be matched but also the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Paolo Gondolo

One aim of cosmic ray measurements is the search for possible signatures of annihilating or decaying dark matter. The so-called positron excess has attracted a lot of attention in this context. On the other hand it has been proposed that…

High Energy Astrophysical Phenomena · Physics 2017-02-02 Rolf Kappl , Annika Reinert

More than a decade ago, the IceCube Neutrino Observatory discovered a diffuse flux of 10 TeV-10 PeV neutrinos from our Universe. This flux of unknown origin most likely emanates from an extragalactic population of neutrino sources, which…

High Energy Astrophysical Phenomena · Physics 2025-06-03 Kathrine Mørch Groth , Markus Ahlers

A model of a lossy nonlinear fiber grating with a "hot spot", which combines a local gain and an attractive perturbation of the refractive index, is introduced. A family of exact solutions for pinned solitons is found in the absence of loss…

Pattern Formation and Solitons · Physics 2009-11-07 William C. K. Mak , Pak L. Chu , Boris A. Malomed