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相关论文: Geodesic motion in the space-time of cosmic string…

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(p,q)-strings are bound states of p F-strings and q D-strings and are predicted to form at the end of brane inflation. As such these cosmic superstrings should be detectable in the universe. In this paper we argue that they can be detected…

高能物理 - 理论 · 物理学 2015-03-17 Betti Hartmann , Claus Lämmerzahl , Parinya Sirimachan

We study the geodesic equation in the space-time of an Abelian-Higgs string and discuss the motion of massless and massive test particles. The geodesics can be classified according to the particles energy, angular momentum and linear…

广义相对论与量子宇宙学 · 物理学 2014-11-21 Betti Hartmann , Parinya Sirimachan

We study the geodesic equation in the space-time of a Kerr black hole pierced by an infinitely thin cosmic string and give the complete set of analytical solutions of this equation for massive and massless particles in terms of Mino time…

广义相对论与量子宇宙学 · 物理学 2014-11-21 Eva Hackmann , Betti Hartmann , Claus Laemmerzahl , Parinya Sirimachan

We study Abelian strings in a fixed de Sitter background. We find that the gauge and Higgs fields extend smoothly across the cosmological horizon and that the string solutions have oscillating scalar fields outside the cosmological horizon…

高能物理 - 理论 · 物理学 2008-11-26 Yves Brihaye , Betti Hartmann

We study the diffusion of massive particles in the space time of an Abelian Higgs string. The particles in the early universe plasma execute Brownian motion. This motion of the particles is modeled as a two dimensional random walk in the…

高能物理 - 唯象学 · 物理学 2018-03-28 Abhisek Saha , Soma Sanyal

We investigate motion of test particles in exact spacetimes with an expanding impulsive gravitational wave which propagates in Minkowski, de Sitter or anti-de Sitter universe. Using the continuous form of these metrics we derive explicit…

广义相对论与量子宇宙学 · 物理学 2010-12-23 Jiri Podolsky , Robert Svarc

We briefly review the equations of motion and the space-time interval due to the nonlinear cosmic string that have been derived in ref. [3] for the first time. The different types of isotropic and nonisotropic geodesic lines in the…

综合物理 · 物理学 2007-05-23 L. M. Chechin , T. B. Omarov

In this paper we analyze Abelian-Higgs strings in a phenomenological model that takes quantum effects in curved space-time into account. This model, first introduced by Rastall, cannot be derived from an action principle. We formulate…

广义相对论与量子宇宙学 · 物理学 2015-06-22 Eugenio R. Bezerra de Mello , Julio C. Fabris , Betti Hartmann

Motivated by astrophysical observations of excess electronic production in the galaxy, new theoretical models of the dark matter sector have been proposed in which the Standard model couples to the dark matter sector through an attractive…

高能物理 - 理论 · 物理学 2009-08-07 Betti Hartmann , Farhad Arbabzadah

We study the geodesic motion of test particles in the space-time of non-compact boson stars. These objects are made of a self-interacting scalar field and -- depending on the scalar field's mass -- can be as dense as neutron stars or even…

广义相对论与量子宇宙学 · 物理学 2013-08-21 Valeria Diemer , Keno Eilers , Betti Hartmann , Isabell Schaffer , Catalin Toma

We study the stability of superconducting strings in a U(1)_{local} x U(1)_{global} model coupled via a gauge field interaction term to U(1) Abelian-Higgs strings. The effect of the interaction on current stability is numerically…

高能物理 - 理论 · 物理学 2013-05-30 Alexandru Babeanu , Betti Hartmann

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…

高能物理 - 唯象学 · 物理学 2016-10-26 Mark Hindmarsh

We report on the energy-momentum correlators obtained with recent numerical simulations of the Abelian Higgs model, essential for the computation of cosmic microwave background and matter perturbations of cosmic strings. Due to significant…

宇宙学与河外天体物理 · 物理学 2017-02-28 David Daverio , Mark Hindmarsh , Martin Kunz , Joanes Lizarraga , Jon Urrestilla

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

We develop a formalism for the quantization of topologically stable excitations in the 4-dimensional abelian lattice gauge theory. The excitations are global and local (Abrikosov-Nielsen-Olesen) strings and monopoles. The operators of…

高能物理 - 格点 · 物理学 2009-10-22 A. K. Bukenov , A. V. Pochinsky , M. I. Polikarpov , L. Polley , U. -J. Wiese

Classical lattice simulations of the Abelian Higgs model are used to investigate small scale structure and loop distributions in cosmic string networks. Use of the field theory ensures that the small-scale physics is captured correctly. The…

高能物理 - 理论 · 物理学 2011-06-02 Mark Hindmarsh , Stephanie Stuckey , Neil Bevis

We derive the geodesic equation of motion in the presence of weak gravitational fields produced by relativistic sources such as cosmic strings, decomposed into scalar, vector and tensor parts. We find that the vector (gravito-magnetic)…

宇宙学与河外天体物理 · 物理学 2012-11-29 Miki Obradovic , Martin Kunz , Mark Hindmarsh , Ilian T. Iliev

We consider the possible existence of gravitationally bound stringlike objects in the framework of the generalized hybrid metric-Palatini gravity theory, in which the gravitational action is represented by an arbitrary function of the Ricci…

广义相对论与量子宇宙学 · 物理学 2021-12-21 Hilberto M. R. da Silva , Tiberiu Harko , Francisco S. N. Lobo , João Luís Rosa

We consider a local cosmic string described by the Abelian-Higgs model in the framework of scalar-tensor gravities. We find the metric of the cosmic string in the weak-field approximation. The propagation of particles and light is analysed…

广义相对论与量子宇宙学 · 物理学 2016-08-15 Maria Emília X. Guimarães

Thermal inflation was proposed as a mechanism to dilute the density of cosmological moduli. Thermal inflation is driven by a complex scalar field possessing a large vacuum expectation value and a very flat potential, called a `flaton'. Such…

宇宙学与河外天体物理 · 物理学 2023-04-13 Robert Brandenberger , Aline Favero
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