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Related papers: Axions from string decay

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This paper revisits the problem of the string decay contribution to the axion cosmological energy density. We show that this contribution is proportional to the average relative increase when axion strings decay of a certain quantity…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. Hagmann , S. Chang , P. Sikivie

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…

Astrophysics · Physics 2009-10-30 R. A. Battye , E. P. S. Shellard

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…

High Energy Physics - Phenomenology · Physics 2026-02-02 Richard A. Battye , Lukasz P. Bunio , Steven J. Cotterill , Pranav B. Gangrekalve Manoj

Cosmological evolution of axionic strings is investigated by numerically solving field equations of a complex scalar field in 3+1 dimensions. It is shown that the global strings relax to the scaling solution with a significantly smaller…

High Energy Physics - Phenomenology · Physics 2009-10-31 Masahide Yamaguchi , M. Kawasaki , Jun'ichi Yokoyama

We study the production of cosmological axions in the standard scenario in which a global string network forms at the Peccei-Quinn phase transition. We make detailed calculations of the axions produced by string loops (a previously…

Astrophysics · Physics 2009-10-22 R. A. Battye , E. P. S. Shellard

We analyze the spectrum of axions radiated from collapse of domain walls, which have received less attention in the literature. The evolution of topological defects related to the axion models is investigated by performing field-theoretic…

High Energy Physics - Phenomenology · Physics 2012-10-17 Takashi Hiramatsu , Masahiro Kawasaki , Ken'ichi Saikawa , Toyokazu Sekiguchi

Cosmic strings formed when the Peccei-Quinn symmetry breaks post-inflation are expected to emit axions throughout their lifetime. The details of the evolution of this network and the associated spectrum of axions are crucial for obtaining…

High Energy Physics - Phenomenology · Physics 2025-12-16 José Correia , Mark Hindmarsh , Joanes Lizarraga , Asier Lopez-Eiguren , Kari Rummukainen , Jon Urrestilla

We study the contribution to the QCD axion dark matter abundance that is produced by string defects during the so-called scaling regime. Clear evidence of scaling violations is found, the most conservative extrapolation of which strongly…

High Energy Physics - Phenomenology · Physics 2021-03-23 Marco Gorghetto , Edward Hardy , Giovanni Villadoro

We discuss the appearance at the QCD phase transition, and the subsequent decay, of axion walls bounded by strings in N=1 axion models. We argue on intuitive grounds that the main decay mechanism is into barely relativistic axions. We…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. Chang , C. Hagmann , P. Sikivie

A generic prediction of string theory is the existence of many axion fields. It has recently been argued that many of these fields should be light and, like the well known QCD axion, lead to observable cosmological consequences. In this…

Cosmology and Nongalactic Astrophysics · Physics 2013-02-19 David J. E. Marsh , Edward Macaulay , Maxime Trebitsch , Pedro G. Ferreira

Axions have for some time been considered a plausible candidate for dark matter. They can be produced through misalignment, but it has been argued that when inflation occurs before a Peccei-Quinn transition, appreciable production can…

High Energy Physics - Phenomenology · Physics 2021-11-22 Michael Dine , Nicolas Fernandez , Akshay Ghalsasi , Hiren H. Patel

Constraints on the tension and the abundance of cosmic strings depend crucially on the rate at which they decay into particles and gravitational radiation. We study the decay of cosmic string loops in the Abelian-Higgs model by performing…

High Energy Physics - Phenomenology · Physics 2019-05-22 Daiju Matsunami , Levon Pogosian , Ayush Saurabh , Tanmay Vachaspati

Axions arise in many theoretical extensions of the Standard Model of particle physics, in particular the "string axiverse". If the axion masses, $m_a$, and (effective) decay constants, $f_a$, lie in specific ranges, then axions contribute…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-18 Matthew J. Stott , David J. E. Marsh , Chakrit Pongkitivanichkul , Layne C. Price , Bobby S. Acharya

Cosmological evolution of axionic string network is analyzed in terms of field-theoretic simulations in a box of 512^3 grids, which are the largest ever, using a new and more efficient identification scheme of global strings. The scaling…

High Energy Physics - Phenomenology · Physics 2011-06-30 Takashi Hiramatsu , Masahiro Kawasaki , Toyokazu Sekiguchi , Masahide Yamaguchi , Jun'ichi Yokoyama

It is shown that the axion concentrated in electroweak strings which are consequently stabilized may produce a rotation of the polarization angle of radiation from extragalactic sources larger than that caused by a background field, and…

Astrophysics · Physics 2011-05-23 Luis Masperi , Sandra Savaglio

A favored scenario for axions to be dark matter is for them to form a cosmic string network that subsequently decays, allowing for a tight link between the axion mass and relic abundance. We discuss an example in which the axion is…

High Energy Physics - Phenomenology · Physics 2024-12-18 James M. Cline , Christos Litos , Wei Xue

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…

Astrophysics · Physics 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…

Astrophysics · Physics 2007-05-23 Elena Melkumova , Dmitry V. Gal'Tsov , Richard Kerner

We study the system of axion strings that forms in the early Universe if the Peccei-Quinn symmetry is restored after inflation. Using numerical simulations, we establish the existence of an asymptotic solution to which the system is…

High Energy Physics - Phenomenology · Physics 2018-08-15 Marco Gorghetto , Edward Hardy , Giovanni Villadoro

Understanding axion cosmology has important experimental consequences since it constrains the range of allowed values for the axion mass. In the standard thermal scenario, which assumes Peccei-Quinn symmetry restoration after inflation, an…

Astrophysics · Physics 2007-05-23 R. A. Battye , E. P. S. Shellard
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