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Related papers: Q-balls: Some Analytical Results

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We discuss various scattering properties of non-topological solitons, Q-balls, on potential obstructions in (1+1) and (2+1) dimensions. These obstructions, barriers and holes, are inserted into the potential of the theory via the coupling…

Mathematical Physics · Physics 2009-05-29 Jassem H. Al-Alawi , Wojtek J. Zakrzewski

In these lecture notes we discuss recent progress in the rigorous derivation of effective evolution equations for the description of the dynamics of quantum mechanical many-body systems.

Mathematical Physics · Physics 2008-07-29 Benjamin Schlein

Analogies between quantum mechanics and sociology lead to the hypothesis that quantum objects are complex products of evolution. Like biological objects they are able to receive, to work on, and to spread semantic information. In general…

Quantum Physics · Physics 2007-05-23 Raoul Nakhmanson

Flat directions in the minimal supersymmetric standard model are known to deform into non-topological solitons, Q-balls, which generally possess both baryon and lepton asymmetries. We investigate how Q-balls evolve if some of the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Masahiro Kawasaki , Fuminobu Takahashi

We construct Q-ball solutions from a model consisting of one massive scalar field $\xi$ and one massive complex scalar field $\phi$ interacting via the cubic couplings $g_1 \xi \phi^{*} \phi + g_2 \xi^3$, typical of Henon-Heiles-like…

High Energy Physics - Theory · Physics 2024-05-01 Y. Brihaye , F. Buisseret

Future experiments may discover new scalar particles with global charges and couplings that allow for solitonic states. If the effective potential has flat directions, the scalar VEV inside a large Q-ball can exceed the particle mass by…

High Energy Physics - Phenomenology · Physics 2009-07-09 Gia Dvali , Alexander Kusenko , Mikhail Shaposhnikov

We investigate how gravity affects Q-balls by exemplifying the case of the Affleck-Dine potential $V(\phi):=m^4 \ln (1+\frac{\phi^2}{m^2})$. Surprisingly, stable Q-balls with arbitrarily small charge exist, no matter how weak gravity is,…

General Relativity and Quantum Cosmology · Physics 2011-09-20 Takashi Tamaki , Nobuyuki Sakai

Rotational excitations of compact Q-balls in the complex signum-Gordon model in 2+1 dimensions are investigated. We find that almost all such spinning Q-balls have the form of a ring of strictly finite width. In the limit of large angular…

High Energy Physics - Theory · Physics 2009-09-24 H. Arodź , J. Karkowski , Z. Świerczyński

We discuss three different globally regular non-topological stationary soliton solutions in the theory of a complex scalar field in 3+1 dimensions, so-called Q-balls, Q-vortices and Q-walls. The charge, energy and profiles of the…

High Energy Physics - Theory · Physics 2015-05-27 Ya Shnir

We study $Q$-ball type solitons in arbitrary spatial dimensions in the setting recently described by Kusenko, where the scalar field potential has a flat direction which rises much slower than $\phi^2$. We find that the general formula for…

High Energy Physics - Theory · Physics 2010-02-03 R. B. MacKenzie , M. B. Paranjape

We study the excited states of the Q-balls by performing stationary perturbation on the spherical Q-balls. We find the exact solution of the stationary perturbation of the global Q-ball with thin wall approximation. For local Q-balls we…

High Energy Physics - Phenomenology · Physics 2009-10-31 Tetsuya Shiromizu , Tomoko Uesugi , Mayumi Aoki

In this study, after introducing algebraic properties of real quaternions some characterizations of quaternionic involute-evolute curves in Q are obtained. And some results and theorems for quaternionic w-curves are given. Lastly, we…

Geometric Topology · Mathematics 2013-11-05 Tülay Soyfidan , Mehmet Ali Güngör

This article gives an overview, aimed at theoretical particle physicists, of some recent developments in cosmology.

High Energy Physics - Phenomenology · Physics 2007-05-23 Andrew R Liddle

The existence of a scaling evolution for cosmic string loops in an expanding universe is demonstrated for the first time by means of numerical simulations. In contrast with what is usually assumed, this result does not rely on any…

Astrophysics · Physics 2009-11-13 Christophe Ringeval , Mairi Sakellariadou , Francois Bouchet

This work considers the algebras of functions in the quantum matrix ball. An explicit formula for a positive invariant integral is presented.

Quantum Algebra · Mathematics 2007-05-23 D. Shklyarov , S. Sinel'shchikov , L. Vaksman

We have made an attempt to compile all currently available data on optically identified QSO absorber systems (Lindner et al. 1996) to establish the status quo of absorber galaxy data as a basis for the investigation of galaxy evolution. We…

Astrophysics · Physics 2016-08-30 Ulrich Lindner , Uta Fritze - von Alvensleben , Klaus J. Fricke

I review recent results for quasars and discuss how they are related to activity in galaxies. Topics included are studies of quasar host galaxies with HST; searches for quasars in the Hubble Deep Field; evolution of the quasar luminosity…

Astrophysics · Physics 2007-05-23 Patrick S. Osmer

Non-topological solitons (Q-balls) are discussed in some stringy settings. Our main result is that the dielectric D-brane system of Myers admits non-abelian Q-ball solutions on their world-volume, in which $N$ D$p$-branes relax to the…

High Energy Physics - Theory · Physics 2016-01-20 Steven Abel , Alex Kehagias

This article, written for Scolarpedia, provides a brief introduction into the subject of cosmic strings, together with a review of their main properties, cosmological evolution and observational signatures.

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Tanmay Vachaspati , Levon Pogosian , Daniele Steer

We examine the energetics of $Q$-balls in Maxwell-Chern-Simons theory in two space dimensions. Whereas gauged $Q$-balls are unallowed in this dimension in the absence of a Chern-Simons term due to a divergent electromagnetic energy, the…

High Energy Physics - Theory · Physics 2013-02-07 M. Deshaies-Jacques , R. MacKenzie