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We describe a thought experiment using an isolated system of known parameters and assuming the correctness of Clausius and Boltzmann descriptions of entropy. The experiment produced an astronomical increase in the number of possible ways…

General Physics · Physics 2007-05-23 Akinbo Ojo

The currently standard theory of cosmic structure formation posits that the present-day clumpy appearance of the universe developed through gravitational amplification of the matter density fluctuations that are generated in the very early…

Astrophysics · Physics 2008-11-26 Naoki Yoshida

We study the formation of cosmic strings by confining a stochastic magnetic field into flux tubes in a numerical simulation. We use overdamped evolution in a potential that is minimized when the flux through each face in the simulation…

High Energy Physics - Theory · Physics 2008-11-26 Jose J. Blanco-Pillado , Ken D. Olum , Alexander Vilenkin

The classical theory of strain in material continua is reviewed and generalized to space-time. Strain is attributed to "external" (matter/energy fields) and intrinsic sources fixing the global symmetry of the universe (defects in the…

General Relativity and Quantum Cosmology · Physics 2010-01-21 Angelo Tartaglia , Ninfa Radicella

We propose that the Universe was created from "Nothing" with a relatively small particles number and it very quick relaxed to quasiequilibrium state at the Planck parameters. The classic cosmological solution for this Universe, with the…

Astrophysics · Physics 2009-10-28 V. Burdyuzha , Yu. Ponomarev , O. Lalaculich , G. Vereshkov

We review current cosmological constraints on the axion. We describe the basic mechanisms by which axions are created in the early universe, focussing on the standard thermal scenario where the dominant process is through axion radiation by…

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

The large-scale structure of the Universe formed from initially small perturbations in the cosmic density field, leading to galaxy clusters with up to 10^15 Msun at the present day. Here, we review the formation of structures in the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-19 S. Planelles , D. R. G. Schleicher , A. M. Bykov

Weinberg relation can be explained by Newton laws. It can also be transformed into a relation between a gravitational cross section area, associated to a gravitational mass m, and the product of two gravitational radii corresponding to the…

General Physics · Physics 2008-06-02 Antonio Alfonso-Faus

Theories with several hundred axion fields have enormous numbers of distinct meta-stable minima. A small fraction of these local minima have vacuum energy compatible with current measurements of dark energy. The potential also contains…

High Energy Physics - Theory · Physics 2019-02-19 Thomas C. Bachlechner , Kate Eckerle , Oliver Janssen , Matthew Kleban

Models of the very early universe, including inflationary models, are argued to produce varying universe domains with different values of fundamental constants and cosmic parameters. Using the cosmological hydrodynamical simulation code…

Cosmology and Nongalactic Astrophysics · Physics 2018-04-10 Luke A. Barnes , Pascal J. Elahi , Jaime Salcido , Richard G. Bower , Geraint F. Lewis , Tom Theuns , Matthieu Schaller , Robert A. Crain , Joop Schaye

Large-scale structure of Universe includes galaxy clusters connected by filaments. Voids occupy the rest of cosmic volume. The search of any dependencities in filament structure can give answer to more general questions about origin of…

Cosmology and Nongalactic Astrophysics · Physics 2019-01-09 V. V. Voitsekhovskiy , A. V. Tugay

Evolution of a universe with homogeneous extra dimensions is studied with the benefit of a well-chosen parameter space that provides a systematic, useful, and convenient way for analysis. In this model we find a natural evolution pattern…

Astrophysics · Physics 2009-11-10 Je-An Gu , W-Y. P. Hwang , Jr-Wei Tsai

We start with the cosmic Friedmann equations, where we adopt a novel perspective rooted in a Lagrangian formulation grounded in Newtonian mechanics and the first law of thermodynamics. Our investigation operates under the assumption that…

General Relativity and Quantum Cosmology · Physics 2024-06-19 Jaume de Haro

Theoretically, the running of the cosmological constant in the IR region is not ruled out. On the other hand, from the QFT viewpoint, the energy released due to the variation of the cosmological constant in the late universe cannot go to…

General Relativity and Quantum Cosmology · Physics 2020-09-30 Jhonny A. Agudelo Ruiz , Tibério de Paula Netto , Júlio C. Fabris , Ilya L. Shapiro

In cosmology it has become usual to introduce new entities as dark matter and dark energy in order to explain otherwise unexplained observational facts. Here, we propose a different approach treating spacetime as a continuum endowed with…

General Relativity and Quantum Cosmology · Physics 2008-11-26 A. Tartaglia , M. Capone

I examine some non-anthropic approaches to the string landscape. These approaches are based on finding the initial conditions of the universe using the wavefunction of the multiverse to select the most probable vacuum out of this landscape.…

High Energy Physics - Theory · Physics 2008-11-26 Edward Tetteh-Lartey

We consider a hypothesis that the closed Universe was formed on the other side of the event horizon of a black hole existing in another universe. That black hole appears in the Universe as a boundary white hole, and its rest frame in…

General Relativity and Quantum Cosmology · Physics 2020-03-03 Nikodem J. Popławski

The structures formation of the Universe appears as if it were a classically self-similar random process at all astrophysical scales. An agreement is demonstrated for the present hypotheses of segregation with a size of astrophysical…

Astrophysics · Physics 2008-11-26 G. Iovane , E. Laserra , F. S. Tortoriello

Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of galaxies tracing the large scale structure (LSS) of the…

Cosmology and Nongalactic Astrophysics · Physics 2019-03-15 P. Daniel Meerburg , Daniel Green , Muntazir Abidi , Mustafa A. Amin , Peter Adshead , Zeeshan Ahmed , David Alonso , Behzad Ansarinejad , Robert Armstrong , Santiago Avila , Carlo Baccigalupi , Tobias Baldauf , Mario Ballardini , Kevin Bandura , Nicola Bartolo , Nicholas Battaglia , Daniel Baumann , Chetan Bavdhankar , José Luis Bernal , Florian Beutler , Matteo Biagetti , Colin Bischoff , Jonathan Blazek , J. Richard Bond , Julian Borrill , François R. Bouchet , Philip Bull , Cliff Burgess , Christian Byrnes , Erminia Calabrese , John E. Carlstrom , Emanuele Castorina , Anthony Challinor , Tzu-Ching Chang , Jonas Chaves-Montero , Xingang Chen , Christophe Yeche , Asantha Cooray , William Coulton , Thomas Crawford , Elisa Chisari , Francis-Yan Cyr-Racine , Guido D'Amico , Paolo de Bernardis , Axel de la Macorra , Olivier Doré , Adri Duivenvoorden , Joanna Dunkley , Cora Dvorkin , Alexander Eggemeier , Stephanie Escoffier , Tom Essinger-Hileman , Matteo Fasiello , Simone Ferraro , Raphael Flauger , Andreu Font-Ribera , Simon Foreman , Oliver Friedrich , Juan Garcia-Bellido , Martina Gerbino , Vera Gluscevic , Garrett Goon , Krzysztof M. Gorski , Jon E. Gudmundsson , Nikhel Gupta , Shaul Hanany , Will Handley , Adam J. Hawken , J. Colin Hill , Christopher M. Hirata , Renée Hložek , Gilbert Holder , Dragan Huterer , Marc Kamionkowski , Kirit S. Karkare , Ryan E. Keeley , William Kinney , Theodore Kisner , Jean-Paul Kneib , Lloyd Knox , Savvas M. Koushiappas , Ely D. Kovetz , Kazuya Koyama , Benjamin L'Huillier , Ofer Lahav , Massimiliano Lattanzi , Hayden Lee , Michele Liguori , Marilena Loverde , Mathew Madhavacheril , Juan Maldacena , M. C. David Marsh , Kiyoshi Masui , Sabino Matarrese , Liam McAllister , Jeff McMahon , Matthew McQuinn , Joel Meyers , Mehrdad Mirbabayi , Azadeh Moradinezhad Dizgah , Pavel Motloch , Suvodip Mukherjee , Julian B. Muñoz , Adam D. Myers , Johanna Nagy , Pavel Naselsky , Federico Nati , Newburgh , Alberto Nicolis , Michael D. Niemack , Gustavo Niz , Andrei Nomerotski , Lyman Page , Enrico Pajer , Hamsa Padmanabhan , Gonzalo A. Palma , Hiranya V. Peiris , Will J. Percival , Francesco Piacentni , Guilherme L. Pimentel , Levon Pogosian , Chanda Prescod-Weinstein , Clement Pryke , Giuseppe Puglisi , Benjamin Racine , Radek Stompor , Marco Raveri , Mathieu Remazeilles , Gracca Rocha , Ashley J. Ross , Graziano Rossi , John Ruhl , Misao Sasaki , Emmanuel Schaan , Alessandro Schillaci , Marcel Schmittfull , Neelima Sehgal , Leonardo Senatore , Hee-Jong Seo , Huanyuan Shan , Sarah Shandera , Blake D. Sherwin , Eva Silverstein , Sara Simon , Anže Slosar , Suzanne Staggs , Glenn Starkman , Albert Stebbins , Aritoki Suzuki , Eric R. Switzer , Peter Timbie , Andrew J. Tolley , Maurizio Tomasi , Matthieu Tristram , Mark Trodden , Yu-Dai Tsai , Cora Uhlemann , Caterina Umilta , Alexander van Engelen , M. Vargas-Magaña , Abigail Vieregg , Benjamin Wallisch , David Wands , Benjamin Wandelt , Yi Wang , Scott Watson , Mark Wise , W. L. K. Wu , Zhong-Zhi Xianyu , Weishuang Xu , Siavash Yasini , Sam Young , Duan Yutong , Matias Zaldarriaga , Michael Zemcov , Gong-Bo Zhao , Yi Zheng , Ningfeng Zhu

A mathematical model of the natural origin of our universe is presented. The model is based only on well-established physics. No claim is made that this model uniquely represents exactly how the universe came about. But the viability of a…

General Relativity and Quantum Cosmology · Physics 2009-04-08 Victor J. Stenger