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We calculate axion radiation emitted in the collision of two straight global strings. The strings are supposed to be in the unexcited ground state, to be inclined with respect to each other, and to move in parallel planes. Radiation arises…

天体物理学 · 物理学 2009-11-10 D. V. Gal'tsov , E. Yu. Melkumova , R. Kerner

A new mechanism of cosmic axion production is proposed: axion bremsstrahlung from collisions of straight global strings. This effect is of the second order in the axion coupling constant, but the resulting cosmological estimate is likely to…

天体物理学 · 物理学 2007-05-23 Elena Melkumova , Dmitry V. Gal'Tsov , Richard Kerner

We consider Cerenkov radiation which must arise when randomly oriented straight cosmic (super)strings move with relativistic velocities without intercommutation. String interactions via dilaton, two-form and gravity (gravity being the…

高能物理 - 理论 · 物理学 2007-05-23 Elena Melkumova , Dmitri Gal'tsov , Karim Salehi

Axions are produced during a period of dilaton-driven inflation by amplification of quantum fluctuations. We show that for some range of string cosmology parameters and some range of axion masses, primordial axions may constitute a large…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

We study early and late time signatures of both QCD axion strings and hyperlight axion strings (axiverse strings). We focus on charge deposition onto axion strings from electromagnetic fields and subsequent novel neutralizing mechanisms due…

高能物理 - 唯象学 · 物理学 2021-05-27 Prateek Agrawal , Anson Hook , Junwu Huang , Gustavo Marques-Tavares

We show that axions can be produced from Abelian-Higgs cosmic strings due to the axion-gauge coupling. The strong magnetic field is confined in the string, and the electric field is induced around the moving string, allowing axion…

高能物理 - 唯象学 · 物理学 2026-04-29 Naoya Kitajima , Michiru Uwabo-Niibo

In the wide variety of axion cosmologies in which axion strings form, their radiative decay is the dominant mechanism for the production of axions, imposing a tight constraint on the axion mass. Here, we focus on the mechanism by which…

天体物理学 · 物理学 2009-10-30 R. A. Battye , E. P. S. Shellard

We have studied numerically the evolution and decay of axion strings. These global defects decay mainly by axion emission and thus contribute to the cosmological axion density. The relative importance of this source relative to misalignment…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Hagmann , S. Chang , P. Sikivie

Low energy string theory predicts the existence of an axion field which can lead to cosmic birefringence. We solve the electromagnetic wave equations in the presence of such an axion and a dilaton field in order to determine their effect on…

高能物理 - 唯象学 · 物理学 2009-10-31 Prasanta Das , Pankaj Jain , Sudipta Mukherji

We discuss key aspects of the nature of radiation from global strings and its impact on the relic axion density. Using a simple model we demonstrate the dependence on the spectrum of radiation emitted by strings. We then study the radiation…

高能物理 - 唯象学 · 物理学 2026-02-02 Richard A. Battye , Lukasz P. Bunio , Steven J. Cotterill , Pranav B. Gangrekalve Manoj

The emission of axions from supernovae is an interesting possibility to account for the Gamma-Ray Bursts provided their energy can be effectively converted into electromagnetic energy elsewhere. The connection between supernova and…

天体物理学 · 物理学 2009-10-31 O. Bertolami

Brane inflation predicts the production of cosmic superstrings with tension 10^{-12}<G\mu<10^{-7}. Superstring theory predicts also the existence of a dilaton with a mass that is at most of the order of the gravitino mass. We show that the…

高能物理 - 理论 · 物理学 2009-11-11 E. Babichev , M. Kachelriess

We develop methods by which cosmic superstring interactions can be studied in detail. These include the reconnection probability and emission of radiation such as gravitons or small string loops. Loop corrections to these are discussed, as…

高能物理 - 理论 · 物理学 2009-11-18 Mark G. Jackson

We consider production of dilepton pairs through coherent electro-magnetic radiation during nuclear collisions. We show that the number of pairs produced through bremsstrahlung is about two orders of magnitude smaller than the yield…

核理论 · 物理学 2008-11-26 J. Jalilian-Marian , V. Koch

The formalism for computing the gravitational power radiation from excitations on cosmic strings forming a junction is presented and applied to the simple case of co-planar strings at a junction when the excitations are generated along one…

高能物理 - 理论 · 物理学 2009-02-12 Robert Brandenberger , Hassan Firouzjahi , Johanna Karouby , Shahram Khosravi

We compute bremsstrahlung arising from the acceleration of individual charged baryons and mesons during the time evolution of high-energy Au+Au collisions at the Relativistic Heavy Ion Collider using a microscopic transport model. We…

高能物理 - 唯象学 · 物理学 2009-10-31 S. M. H. Wong , M. Belkacem , J. I. Kapusta , S. A. Bass , M. Bleicher , H. Stöcker

We review current cosmological constraints on the axion. We describe the basic mechanisms by which axions are created in the early universe, focussing on the standard thermal scenario where the dominant process is through axion radiation by…

天体物理学 · 物理学 2016-08-30 R. A. Battye , E. P. S. Shellard

The current cosmological constraints on a dark matter axion are reviewed. We describe the basic mechanisms by which axions are created in the early universe, both in the standard thermal scenario in which axion strings form and in…

天体物理学 · 物理学 2016-10-26 E. P. S. Shellard , R. A. Battye

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

Axion is a promising candidate of dark matter in the universe. A fraction of dark matter axion may forms axion star with radius $\sim 10^2$km. We show that the axion star emits radiation burst by the collision with K and M types main…

高能物理 - 唯象学 · 物理学 2022-04-20 Aiichi Iwazaki
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