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Related papers: Multimodal axion emissions from Abelian-Higgs cosm…

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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

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…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ram Brustein , Merav Hadad

Dark photon dark matter may be produced by the cosmic strings in association with the dark U(1) gauge symmetry breaking. We perform three-dimensional lattice simulations of the Abelian-Higgs model and follow the evolution of cosmic strings.…

High Energy Physics - Phenomenology · Physics 2023-08-04 Naoya Kitajima , Kazunori Nakayama

Axions seem ubiquitous in string theories and some of them may be produced non-thermally by heavy scalar decays, contributing to dark radiation. We study various cosmological effects of photons produced from the axionic dark radiation…

High Energy Physics - Phenomenology · Physics 2015-06-16 Tetsutaro Higaki , Kazunori Nakayama , Fuminobu Takahashi

Axions have long been considered plausible candidates for dark matter. The axion dark matter emitted from cosmic strings after the Peccei-Quinn (PQ) symmetry breaking in the early Universe was extensively simulated. In this work, we study…

High Energy Physics - Phenomenology · Physics 2025-04-02 Yongtao Jia , Ligong Bian

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…

Astrophysics · Physics 2016-10-26 E. P. S. Shellard , R. A. Battye

We evaluate the efficiency of axion production from spatially random initial conditions in the axion field, so a network of axionic strings is present. For the first time, we perform numerical simulations which fully account for the large…

High Energy Physics - Phenomenology · Physics 2017-12-13 Vincent B. Klaer , Guy D. Moore

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

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

A generic low-energy prediction of string theory is the existence of a large collection of axions, commonly known as a string axiverse. Axions also have a natural cosmological production mechanism, vacuum misalignment, making them…

High Energy Physics - Phenomenology · Physics 2022-03-22 David Cyncynates , Tudor Giurgica-Tiron , Olivier Simon , Jedidiah O. Thompson

Axions constitute a well-motivated dark matter candidate, and if PQ symmetry breaking occurred after inflation, it should be possible to make a clean prediction for the relation between the axion mass and the axion dark matter density. We…

High Energy Physics - Phenomenology · Physics 2016-01-13 Leesa Fleury , Guy D. Moore

We numerically study string production by evolving classical Abelian-Higgs gauge field wavepackets. Initial conditions are constructed for the propagation of a single wavepacket and for the collision of two wavepackets. We identify regions…

High Energy Physics - Theory · Physics 2019-05-15 Ayush Saurabh , Tanmay Vachaspati

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

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 discuss the possible sources of dark matter axions in the early universe. In the standard thermal scenario, an axion string network forms at the Peccei-Quinn phase transition $T\sim \fa$ and then radiatively decays into a cosmological…

Astrophysics · Physics 2016-08-30 E. P. S. Shellard , R. A. Battye

We discuss a possible principle for detecting dark matter axions in galactic halos. If axions constitute a condensate in the Milky Way, stimulated emissions of the axions from a type of excitation in condensed matter can be detectable. We…

High Energy Physics - Phenomenology · Physics 2017-01-30 Naoto Yokoi , Eiji Saitoh

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 perform the lattice simulation to estimate the axion dark matter abundance radiated from the global cosmic strings in the post-inflationary scenario. The independent numerical confirmation on the recently observed logarithmic growth in…

High Energy Physics - Phenomenology · Physics 2024-07-17 Heejoo Kim , Junghyeon Park , Minho Son

In the string axiverse scenario, light primordial black holes may spin up due to the Hawking emission of a large number of light (sub-MeV) axions. We show that this may trigger superradiant instabilities associated with a heavier axion…

High Energy Physics - Phenomenology · Physics 2023-06-19 Marco Calzà , João G. Rosa , Filipe Serrano

I report on recent numerical simulations of the simplest field theory with cosmic string solutions, the Abelian Higgs model. We find that random networks of string quickly converge to a scaling solution in which the network scale length…

High Energy Physics - Phenomenology · Physics 2016-10-26 Mark Hindmarsh
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