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相关论文: Cosmic Rays From Cosmic Strings

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We re-visit the production of cosmic rays by cusps on cosmic strings. If a scalar field (``Higgs'') has a linear interaction with the string world-sheet, such as would occur if there is a bosonic condensate on the string, cusps on string…

宇宙学与河外天体物理 · 物理学 2014-11-20 Tanmay Vachaspati

The topological defect scenario of origin of the observed highest energy cosmic rays is reviewed. Under a variety of circumstances, topological defects formed in the early Universe can be sources of very massive particles in the Universe…

天体物理学 · 物理学 2009-10-30 Pijushpani Bhattacharjee

We calculate the flux of ultra high energy photons from individual ordinary (i.e. non-superconducting) cosmic strings and compare the results with the sensitivity of current and proposed TeV and EeV telescopes. Our calculations give only…

天体物理学 · 物理学 2009-10-22 Jane H. MacGibbon , Robert H. Brandenberger

It is shown that the fusion of strings is a source of particle production in nucleus--nucleus collisions outside the kinematical limits of nucleon--nucleon collisions. This fact, together with another effect of string fusion, the reduction…

高能物理 - 唯象学 · 物理学 2009-10-28 N. Armesto , M. A. Braun , E. G. Ferreiro , C. Pajares , Yu. M. Shabelski

Cosmic strings are topological defects possibly formed in the early Universe, which may be observable due to their gravitational effects on the cosmic microwave background radiation or gravitational wave experiments. To this effect it is…

宇宙学与河外天体物理 · 物理学 2017-03-01 R. P. L. Azevedo , C. J. A. P. Martins

We give an upper estimate for the number of gamma ray bursts from ordinary (non-superconducting) cosmic strings expected to be observed at terrestrial detectors. Assuming that cusp annihilation is the mechanism responsible for the bursts we…

高能物理 - 唯象学 · 物理学 2016-09-01 R. H. Brandenberger , A. T. Sornborger , M. Trodden

A synthesis of previous work done on the microscopic structure of cosmic strings in realistic models is made and reveals that strings are expected to be not only superconducting in the sense of Witten, but also generically current-carrying,…

高能物理 - 唯象学 · 物理学 2009-10-28 Anne-Christine Davis , Patrick Peter

Topological defects, particularly cosmic strings, can provide a mechanism to produce particles with energies of the order 10^21 eV and higher. Here, we report on order of magnitude calculations of fluxes from a cosmic string network which…

高能物理 - 唯象学 · 物理学 2007-05-23 U. F. Wichoski , R. H. Brandenberger , J. H. MacGibbon

It has been suggested that cosmological gamma-ray bursts (GRBs) can produce the observed flux of cosmic rays at the highest energies. However, recent studies of GRBs indicate that their redshift distribution likely follows that of the…

天体物理学 · 物理学 2009-10-31 S. T. Scully , F. W. Stecker

The flux of high energy cosmic rays coming from the decay of vortons is estimated. If the abundance of loops corresponding to a superconductivity scale coincident with that of the string formation is corrected to be compatible with the…

天体物理学 · 物理学 2011-05-23 Luis Masperi , Guillermo Silva

Making use of the wealth of new observational data coming from the sky it is possible to constrain particle physics theories beyond the Standard Model. One way to do this is illustrated in this article: a subset of theories admits cosmic…

宇宙学与河外天体物理 · 物理学 2014-01-21 Robert H. Brandenberger

Decaying topological defects, in particular cosmic strings, can produce a significant flux of high energy neutrinos, photons and cosmic rays. According to the prevailing understanding of cosmic string dynamics in an expanding Universe, the…

高能物理 - 唯象学 · 物理学 2009-10-31 Ubi F. Wichoski , Jane H. MacGibbon , Robert H. Brandenberger

The formation of cusps on long cosmic strings is discussed and the probability of cusp formation is estimated. The energy distribution of the gamma-ray background due to cusp annihilation on long strings is calculated and compared to…

高能物理 - 唯象学 · 物理学 2009-10-22 M. Mohazzab , R. H. Brandenberger

We calculate the gravitational radiation emitted by an infinite cosmic string with two oppositely moving wave-trains, in the small amplitude approximation. After comparing our result to the previously studied cases we extend the results to…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Xavier Siemens , Ken D. Olum

Understanding of the signatures of cosmic string networks is limited by a large uncertainty in the sizes at which cosmic string loops form. We review cosmic string network evolution, and the gravitational signatures, with emphasis on this…

天体物理学 · 物理学 2007-11-07 Joseph Polchinski

The origin of cosmic rays is one of the major unresolved astrophysical questions. In particular, the highest energy cosmic rays observed possess macroscopic energies and their origin is likely to be associated with the most energetic…

天体物理学 · 物理学 2007-05-23 Guenter Sigl

We study the spectrum of cosmic ray positrons produced by a scaling distribution of non-superconducting cosmic strings. In this scenario, the positrons are produced from the jets which form from the cosmic string cusp annihilation process.…

高能物理 - 唯象学 · 物理学 2009-01-25 Robert Brandenberger , Yi-Fu Cai , Wei Xue , Xinmin Zhang

The origin of cosmic rays is one of the major unresolved questions in astrophysics. In particular, the highest energy cosmic rays observed possess macroscopic energies and their origin is likely associated with the most energetic processes…

天体物理学 · 物理学 2009-11-06 Guenter Sigl

We consider the cosmological consequences of a network of superconducting cosmic strings. For strong enough current the period of friction domination never ends. Instead a plasma scaling solution is reached. We demonstrate that this gives…

高能物理 - 唯象学 · 物理学 2009-10-31 K. Dimopoulos , A. C. Davis

The time-dependent metric of a cosmic string leads to an effective interaction between the string and photons - the "gravitational Aharonov-Bohm" effect -- and causes cosmic strings to emit light. We evaluate the radiation of pairs of…

高能物理 - 理论 · 物理学 2011-03-23 Daniele A. Steer , Tanmay Vachaspati
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