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Brane inflation in superstring theory predicts that cosmic strings (but not domain walls or monopoles) are produced towards the end of the inflationary epoch. Here, we discuss the production, the spectrum and the evolution of such cosmic…

High Energy Physics - Theory · Physics 2009-11-10 Nicholas T. Jones , Horace Stoica , S. -H. Henry Tye

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

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 consider the Schwinger production of baryons in an external electric field in the worldline instanton approach. The process occurs in the confinement regime hence the holographic QCD and the Chiral Lagrangian are used as the tools. The…

High Energy Physics - Theory · Physics 2023-12-08 Alexander Gorsky , Arseniy Pikalov

There exists a class of cosmic strings that turn matter into antimatter (Alice strings). In a GUT where the unbroken gauge group contains charge conjugation ($C$), such strings form when a phase transition renders $C$ a discrete symmetry.…

High Energy Physics - Phenomenology · Physics 2016-09-01 Shahar Ben-Menahem , Adrian R. Cooper

In a $\Lambda$CDM cosmology, galaxy formation is a globally inefficient process: it is often the case that far fewer baryons are observed in galaxy disks than expected from the cosmic baryon fraction. The location of these "missing baryons"…

Astrophysics of Galaxies · Physics 2018-08-15 Harley Katz , Harry Desmond , Federico Lelli , Stacy McGaugh , Arianna Di Cintio , Chris Brook , James Schombert

A fluid of Skyrmions coupled to the dilaton field and the $\o$ meson field is considered. A mean field theory is developed in which the dilaton and the $\o$ field acquire a mean value determined by the Skyrmions. The influence of the…

High Energy Physics - Phenomenology · Physics 2016-09-06 G. Kälbermann

Skyrmions are stable and topologically non-trivial field configurations that behave like localized particles. They appear in the chiral effective theory for pions, where they correspond to the baryon states, and might also exist in the…

High Energy Physics - Phenomenology · Physics 2026-01-28 Mikael Chala , Juan Carlos Criado , Luis Gil

Near threshold neutral pion electroproduction on the deuteron is studied in the framework of heavy baryon chiral perturbation theory. We include the next-to-leading order corrections to the three-body contributions. We find an improved…

Nuclear Theory · Physics 2007-05-23 H. Krebs , V. Bernard , Ulf-G. Meißner

A compelling production mechanism for QCD axion dark matter is from the scaling dynamics of early universe axion strings. We show that in DFSZ-like models containing tree-level interactions between fermions and the axion, friction between…

High Energy Physics - Phenomenology · Physics 2026-03-03 Anson Hook , Rajrupa Mondal , Shourya Mukherjee

We study quantum corrections at the one loop level in open superstring tachyon condensation using the boundary string field theory (BSFT) method. We find that the tachyon field action has the same form as at the disc level, but with a…

High Energy Physics - Theory · Physics 2009-11-07 K. S. Viswanathan , Y. Yang

Recent experimental data on antibaryon production outside nucleon-nucleon kinematical limits have been obtained in Pb-Pb collisions at SPS energies. We present a possible explanation for this phenomenon based on the existence of collective…

High Energy Physics - Phenomenology · Physics 2007-05-23 E. G. Ferreiro , C. Pajares

Brane inflation in superstring theory ends when branes collide, initiating the hot big bang. Cosmic superstrings are produced during the brane collision. The cosmic superstrings produced in a D3-brane-antibrane inflationary scenario have a…

Astrophysics · Physics 2014-10-13 S. -H. Henry Tye , Ira Wasserman , Mark Wyman

The process of secondary baryon production in pi(+-)p collisions at high energies in the central and forward fragmentation regions is considered in the framework of the Quark-Gluon String Model. The contribution of the string-junction…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. H. Arakelyan , C. Merino , Yu. M. Shabelski

We investigate the pair creation of magnetically charged black holes on a cosmic string in the presence of a background magnetic field. The string may either break or fray to produce a pair of accelerating black holes described by Ernst…

High Energy Physics - Theory · Physics 2021-03-24 Amjad Ashoorioon , Mohammad Bagher Jahani Poshteh

Fundamental superstrings (F-strings) and D-strings may be produced at high temperature in the early Universe. Assuming that, we investigate if any of the instabilities present in systems of strings and branes can give rise to a…

High Energy Physics - Theory · Physics 2008-11-26 J. L. Cornou , E. Pajer , R. Sturani

We introduce a novel Skyrme-like conserved current in the effective theory of pions and vector mesons based on the idea of hidden local symmetry. The associated charge is equivalent to the skyrmion charge for any smooth configuration. In…

High Energy Physics - Theory · Physics 2020-07-22 Avner Karasik

We construct nontopological string solutions with U(1) Noether charge in the Skyrme model with a pion mass term, and examine their stability by taking linear perturbations. The solution exhibits a critical angular velocity beyond which the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Muneto Nitta , Noriko Shiiki

Recent developments in string inspired models of inflation suggest that D-strings are formed at the end of inflation. Within the supergravity model of D-strings there are 2(n-1) chiral fermion zero modes for a D-string of winding n. Using…

High Energy Physics - Theory · Physics 2008-11-26 Ph. Brax , C. van de Bruck , A. C. Davis , Stephen C. Davis

Recent studies suggest that the process of symmetry breaking after inflation typically occurs very fast, within a single oscillation of the symmetry-breaking field, due to the spinodal growth of its long-wave modes, otherwise known as…

High Energy Physics - Phenomenology · Physics 2009-11-07 Juan Garcia-Bellido , Ester Ruiz Morales