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Large-scale accretion shocks around massive clusters of galaxies, generically expected in hierarchical scenarios of cosmological structure formation, are shown to be potential sources of the observed ultrahigh energy cosmic rays (UHECRs) by…

Astrophysics · Physics 2007-11-08 Susumu Inoue , Guenter Sigl , Francesco Miniati , Eric Armengaud

Ultra-high energy cosmic rays are mostly charged particles and they are therefore deflected by magnetic fields on their path from their sources to Earth. An interesting phenomenon arising from these deflections is the appearance of multiple…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Geraldina Golup , Diego Harari , Silvia Mollerach , Esteban Roulet

In this paper we investigate the electrodynamic surface properties of bare strange quark stars. The surfaces of such objects are characterized by the formation of ultra-high electric surface fields which might be as high as $\sim 10^{19}$…

High Energy Astrophysical Phenomena · Physics 2010-12-23 Rodrigo Picanço Negreiros , Igor N. Mishustin , Stefan Schramm , Fridolin Weber

Ultra high energy cosmic ray events presently show a spectrum, which we interpret here as galactic cosmic rays due to a starburst in the radio galaxy Cen A pushed up in energy by the shock of a relativistic jet. The knee feature and the…

High Energy Astrophysical Phenomena · Physics 2010-11-02 P. L. Biermann , J. K. Becker , L. Caramete , L. A. Gergely , I. C. Maris , A. Meli , V. de Souza , T. Stanev

We discuss the possible imprints of strangelets (i.e., lumps of Strange Quark Matter) in Chacaltaya experimental data using model of propagation of such objects through the atmosphere developed by us recently.

High Energy Physics - Phenomenology · Physics 2010-11-11 M. Rybczynski , Z. Wlodarczyk , G. Wilk

Pulsar-like objects are extremely compact, with an average density that exceeds nuclear saturation density, where the fundamental strong interaction plays an essential role, particularly in the low-energy regime. The internal structures and…

High Energy Astrophysical Phenomena · Physics 2025-11-04 Chengjun Xia , Xiaoyu Lai , Renxin Xu

Strange stars are one of the hypothetical compact stellar objects that can be formed after a supernova explosion. The existence of these objects relies on the absolute stability of strange {\it collapsed} quark matter with respect to…

High Energy Astrophysical Phenomena · Physics 2014-11-26 Massimo Mannarelli

Neutron stars have long been regarded as extra-terrestrial laboratories from which we can learn about extreme energy density matter at low temperatures. In this article, I highlight some of the recent advances made in astrophysical…

Solar and Stellar Astrophysics · Physics 2023-07-19 Madappa Prakash

The origin of the highest energy cosmic rays is still unknown. The discovery of their sources will reveal the workings of the most energetic astrophysical accelerators in the universe. Current observations show a spectrum consistent with an…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Kumiko Kotera , Angela V. Olinto

Strange quark matter (SQM) may be the true ground state of matter. According to this SQM hypothesis, the observed neutron stars actually should all be strange quark stars. But distinguishing between neutron stars and strange quark stars by…

High Energy Astrophysical Phenomena · Physics 2021-10-01 Xu Wang , Yong-Feng Huang , Bing Li

We study the partial fragmentation of a strange quark star into strangelets during the process of merger of two strange quark stars. We discuss the fate of the fragments considering their possible evaporation into nucleons. We show that…

High Energy Astrophysical Phenomena · Physics 2022-11-09 Niccolò Bucciantini , Alessandro Drago , Giuseppe Pagliara , Silvia Traversi , Andreas Bauswein

We review the physics of the highest energy cosmic rays. The discovery of their sources, still unknown, will reveal the most energetic astrophysical objects in the universe and could unveil new physics beyond the standard model of particle…

High Energy Astrophysical Phenomena · Physics 2017-11-30 Roberto Aloisio

In this paper intergalatic electromagnetic cascades are used as a probe of cosmic ray sources. This is achieved as follows. In extragalactic space cosmic rays initiate electromagnetic cascades in which gamma-ray and neutrino emission…

High Energy Astrophysical Phenomena · Physics 2022-12-01 Anna Uryson

It is now widely acknowledged that cosmic rays experiments can test possible new physics directly generated at the Planck scale or at some other fundamental scale. By studying particle properties at energies far beyond the reach of any…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Luis Gonzalez-Mestres

Quark nuggets are theoretical objects composed of approximately equal numbers of up, down, and strange quarks. They are also called strangelets, nuclearites, AQNs, slets, Macros, and MQNs. Quark nuggets are a candidate for dark matter,…

High Energy Astrophysical Phenomena · Physics 2020-09-30 J. Pace VanDevender , C. Jerald Buchenauer , Chunpei Cai , Aaron P. VanDevender , Benjamin A. Ulmen

The propagation of ultra high energy cosmic rays in Galactic and extragalactic magnetic fields is investigated in the present paper. The motion of charged particles of different energies and chemical composition is simulated using different…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Oleksandr Sushchov , Oleh Kobzar , Bohdan Hnatyk , Volodymyr Marchenko

Some general features of cosmic ray acceleration are summarized along with some inferences that can be drawn concerning the origin of the UHE component. The UHE luminosity density is found to be similar to that derived for GeV cosmic rays…

Astrophysics · Physics 2010-12-03 R. D. Blandford

It is shown that extremely strong electric fields may be generated at the surface of strange quark matter in the color-flavor locked phase because of the surface effects. Some properties of strange stars made of this matter are briefly…

Astrophysics · Physics 2009-11-10 V. V. Usov

The properties of strange quark matter and strange hadronic matter and their finite counterparts (strangelets and MEMOs) are reviewed. The production of strange matter in heavy-ion collision and the appearance of strange matter in neutron…

Nuclear Theory · Physics 2009-09-25 Carsten Greiner , Juergen Schaffner-Bielich

As many as $10^9$ neutron stars populate the Galaxy, but only $\approx 10^3$ are directly observed as pulsars or as accreting sources in X-ray binaries. In principle also the accretion of the interstellar medium may make isolated neutron…

Astrophysics · Physics 2009-10-31 Aldo Treves , Roberto Turolla , Silvia Zane , Monica Colpi
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