Zobrazeno 1 - 10
of 448
pro vyhledávání: '"Peter Mészáros"'
Autor:
He Gao, Peter Mészáros
Publikováno v:
Advances in Astronomy, Vol 2015 (2015)
A generic synchrotron external shock model is the widely preferred paradigm used to interpret the broadband afterglow data of gamma-ray bursts (GRBs), including predicted observable signatures from a reverse shock which have been confirmed by observa
Externí odkaz:
https://doaj.org/article/c20f55a4105b49fbb3d4517ee918e115
Autor:
Péter Mészáros
In the last two decades, cosmology, particle physics, high energy astrophysics and gravitational physics have become increasingly interwoven. The intense activity taking place at the intersection of these disciplines is constantly progressing, with t
Autor:
Geoffrey C. Bower, Conor Omand, D. B. Fox, R. Margutti, Kohta Murase, Ryan Chornock, Hiroshi Nagai, Deanne L. Coppejans, Casey J. Law, Peter Mészáros, Kazumi Kashiyama
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 508:44-51
Fast-rotating pulsars and magnetars have been suggested as the central engines of super-luminous supernovae (SLSNe) and fast radio bursts, and this scenario naturally predicts non-thermal synchrotron emission from their nascent pulsar wind nebulae (P
Autor:
Peter Mészáros, Peter Meszaros
Publikováno v:
The Fifteenth Marcel Grossmann Meeting.
Solid inflation is a cosmological model where inflation is driven by fields which enter the Lagrangian in the same way as body coordinates of a solid matter enter the equation of state, spontaneously breaking spatial translational and rotational symm
Autor:
A. Tohuvavohu, Emily Calamari, Kohta Murase, Phil Evans, Alexis Coleiro, Marcos Santander, Peter Mészáros, D. B. Fox, Azadeh Keivani, J. A. Kennea, Thomas D. Russell, Felicia Krauß
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 497 (3), pp.2553-2561. ⟨10.1093/mnras/staa2148⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 497 (3), pp.2553-2561. ⟨10.1093/mnras/staa2148⟩
Monthly Notices of the Royal Astronomical Society, 497(3), 2553-2561. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 2020, 497 (3), pp.2553-2561. ⟨10.1093/mnras/staa2148⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 497 (3), pp.2553-2561. ⟨10.1093/mnras/staa2148⟩
Monthly Notices of the Royal Astronomical Society, 497(3), 2553-2561. Oxford University Press
High-energy neutrinos are a promising tool for identifying astrophysical sources of high and ultra-high energy cosmic rays (UHECR). Prospects of detecting neutrinos at high energies ($\gtrsim$TeV) from blazars have been boosted after the recent assoc
Publikováno v:
Nature Reviews Physics. 1:585-599
Multi-messenger astrophysics, a long-anticipated extension to traditional and multiwavelength astronomy, has recently emerged as a distinct discipline providing unique and valuable insights into the properties and processes of the physical universe.
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 489:4347-4366
Motivated by the recently reported evidence of an association between a high-energy neutrino and a gamma-ray flare from the blazar TXS 0506+056, we calculate the expected high-energy neutrino signal from past, individual flares, from twelve blazars,
Autor:
Peter Mészáros
Publikováno v:
Debreceni Jogi Műhely. 17
As a powerful source of gravitational waves (GW), a supermassive black hole (SMBH) merger may be accompanied by a relativistic jet that leads to detectable electromagnetic (EM) emission. We model the propagation of post-merger jets inside a pre-merge
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e638969694719b8376320c733fe3b7c
http://arxiv.org/abs/2101.05788
http://arxiv.org/abs/2101.05788
The recent detection of TeV photons from two gamma-ray bursts (GRBs), GRB 190114C and GRB 180720B, has opened a new window for multi-messenger and multi-wavelength astrophysics of high-energy transients. We study the origin of very-high-energy (VHE)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb4c2ef81c64fd2399854ee3844990b0
http://arxiv.org/abs/2012.09143
http://arxiv.org/abs/2012.09143