Thermodynamics of Cosmological Matter Creation I
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Arxiv:1904.10313V3 [Gr-Qc] 22 Oct 2020 PACS Numbers: Keywords: Entropy, Holographic Principle and CCDM Models
Thermodynamic constraints on matter creation models R. Valentim∗ Departamento de F´ısica, Instituto de Ci^enciasAmbientais, Qu´ımicas e Farmac^euticas - ICAQF, Universidade Federal de S~aoPaulo (UNIFESP) Unidade Jos´eAlencar, Rua S~aoNicolau No. 210, 09913-030 { Diadema, SP, Brazil J. F. Jesusy Universidade Estadual Paulista (UNESP), C^ampusExperimental de Itapeva Rua Geraldo Alckmin 519, 18409-010, Vila N. Sra. de F´atima,Itapeva, SP, Brazil and Universidade Estadual Paulista (UNESP), Faculdade de Engenharia de Guaratinguet´a Departamento de F´ısica e Qu´ımica, Av. Dr. Ariberto Pereira da Cunha 333, 12516-410 - Guaratinguet´a,SP, Brazil Abstract Entropy is a fundamental concept from Thermodynamics and it can be used to study models on context of Creation Cold Dark Matter (CCDM). From conditions on the first (S_ 0)1 and ≥ second order (S¨ < 0) time derivatives of total entropy in the initial expansion of Sitter through the radiation and matter eras until the end of Sitter expansion, it is possible to estimate the intervals of parameters. The total entropy (St) is calculated as sum of the entropy at all eras (Sγ and Sm) plus the entropy of the event horizon (Sh). This term derives from the Holographic Principle where it suggests that all information is contained on the observable horizon. The main feature of this method for these models are that thermodynamic equilibrium is reached in a final de Sitter era. Total entropy of the universe is calculated with three terms: apparent horizon (Sh), entropy of matter (Sm) and entropy of radiation (Sγ). This analysis allows to estimate intervals of parameters of CCDM models. -
Birth of De Sitter Universe from a Time Crystal Universe
PHYSICAL REVIEW D 100, 123531 (2019) Birth of de Sitter universe from a time crystal universe † Daisuke Yoshida * and Jiro Soda Department of Physics, Kobe University, Kobe 657-8501, Japan (Received 30 September 2019; published 18 December 2019) We show that a simple subclass of Horndeski theory can describe a time crystal universe. The time crystal universe can be regarded as a baby universe nucleated from a flat space, which is mediated by an extension of Giddings-Strominger instanton in a 2-form theory dual to the Horndeski theory. Remarkably, when a cosmological constant is included, de Sitter universe can be created by tunneling from the time crystal universe. It gives rise to a past completion of an inflationary universe. DOI: 10.1103/PhysRevD.100.123531 I. INTRODUCTION Euler-Lagrange equations of motion contain up to second order derivatives. Actually, bouncing cosmology in the Inflation has succeeded in explaining current observa- Horndeski theory has been intensively investigated so far tions of the large scale structure of the Universe [1,2]. [23–29]. These analyses show the presence of gradient However, inflation has a past boundary [3], which could be instability [30,31] and finally no-go theorem for stable a true initial singularity or just a coordinate singularity bouncing cosmology in Horndeski theory was found for the depending on how much the Universe deviates from the spatially flat universe [32]. However, it was shown that the exact de Sitter [4], or depending on the topology of the no-go theorem does not hold when the spatial curvature is Universe [5]. -
Expanding Space, Quasars and St. Augustine's Fireworks
Universe 2015, 1, 307-356; doi:10.3390/universe1030307 OPEN ACCESS universe ISSN 2218-1997 www.mdpi.com/journal/universe Article Expanding Space, Quasars and St. Augustine’s Fireworks Olga I. Chashchina 1;2 and Zurab K. Silagadze 2;3;* 1 École Polytechnique, 91128 Palaiseau, France; E-Mail: [email protected] 2 Department of physics, Novosibirsk State University, Novosibirsk 630 090, Russia 3 Budker Institute of Nuclear Physics SB RAS and Novosibirsk State University, Novosibirsk 630 090, Russia * Author to whom correspondence should be addressed; E-Mail: [email protected]. Academic Editors: Lorenzo Iorio and Elias C. Vagenas Received: 5 May 2015 / Accepted: 14 September 2015 / Published: 1 October 2015 Abstract: An attempt is made to explain time non-dilation allegedly observed in quasar light curves. The explanation is based on the assumption that quasar black holes are, in some sense, foreign for our Friedmann-Robertson-Walker universe and do not participate in the Hubble flow. Although at first sight such a weird explanation requires unreasonably fine-tuned Big Bang initial conditions, we find a natural justification for it using the Milne cosmological model as an inspiration. Keywords: quasar light curves; expanding space; Milne cosmological model; Hubble flow; St. Augustine’s objects PACS classifications: 98.80.-k, 98.54.-h You’d think capricious Hebe, feeding the eagle of Zeus, had raised a thunder-foaming goblet, unable to restrain her mirth, and tipped it on the earth. F.I.Tyutchev. A Spring Storm, 1828. Translated by F.Jude [1]. 1. Introduction “Quasar light curves do not show the effects of time dilation”—this result of the paper [2] seems incredible. -
European Astroparticle Physics Strategy 2017-2026 Astroparticle Physics European Consortium
European Astroparticle Physics Strategy 2017-2026 Astroparticle Physics European Consortium August 2017 European Astroparticle Physics Strategy 2017-2026 www.appec.org Executive Summary Astroparticle physics is the fascinating field of research long-standing mysteries such as the true nature of Dark at the intersection of astronomy, particle physics and Matter and Dark Energy, the intricacies of neutrinos cosmology. It simultaneously addresses challenging and the occurrence (or non-occurrence) of proton questions relating to the micro-cosmos (the world decay. of elementary particles and their fundamental interactions) and the macro-cosmos (the world of The field of astroparticle physics has quickly celestial objects and their evolution) and, as a result, established itself as an extremely successful endeavour. is well-placed to advance our understanding of the Since 2001 four Nobel Prizes (2002, 2006, 2011 and Universe beyond the Standard Model of particle physics 2015) have been awarded to astroparticle physics and and the Big Bang Model of cosmology. the recent – revolutionary – first direct detections of gravitational waves is literally opening an entirely new One of its paths is targeted at a better understanding and exhilarating window onto our Universe. We look of cataclysmic events such as: supernovas – the titanic forward to an equally exciting and productive future. explosions marking the final evolutionary stage of massive stars; mergers of multi-solar-mass black-hole Many of the next generation of astroparticle physics or neutron-star binaries; and, most compelling of all, research infrastructures require substantial capital the violent birth and subsequent evolution of our infant investment and, for Europe to remain competitive Universe. -
On Asymptotically De Sitter Space: Entropy & Moduli Dynamics
On Asymptotically de Sitter Space: Entropy & Moduli Dynamics To Appear... [1206.nnnn] Mahdi Torabian International Centre for Theoretical Physics, Trieste String Phenomenology Workshop 2012 Isaac Newton Institute , CAMBRIDGE 1 Tuesday, June 26, 12 WMAP 7-year Cosmological Interpretation 3 TABLE 1 The state of Summarythe ofart the cosmological of Observational parameters of ΛCDM modela Cosmology b c Class Parameter WMAP 7-year ML WMAP+BAO+H0 ML WMAP 7-year Mean WMAP+BAO+H0 Mean 2 +0.056 Primary 100Ωbh 2.227 2.253 2.249−0.057 2.255 ± 0.054 2 Ωch 0.1116 0.1122 0.1120 ± 0.0056 0.1126 ± 0.0036 +0.030 ΩΛ 0.729 0.728 0.727−0.029 0.725 ± 0.016 ns 0.966 0.967 0.967 ± 0.014 0.968 ± 0.012 τ 0.085 0.085 0.088 ± 0.015 0.088 ± 0.014 2 d −9 −9 −9 −9 ∆R(k0) 2.42 × 10 2.42 × 10 (2.43 ± 0.11) × 10 (2.430 ± 0.091) × 10 +0.030 Derived σ8 0.809 0.810 0.811−0.031 0.816 ± 0.024 H0 70.3km/s/Mpc 70.4km/s/Mpc 70.4 ± 2.5km/s/Mpc 70.2 ± 1.4km/s/Mpc Ωb 0.0451 0.0455 0.0455 ± 0.0028 0.0458 ± 0.0016 Ωc 0.226 0.226 0.228 ± 0.027 0.229 ± 0.015 2 +0.0056 Ωmh 0.1338 0.1347 0.1345−0.0055 0.1352 ± 0.0036 e zreion 10.4 10.3 10.6 ± 1.210.6 ± 1.2 f t0 13.79 Gyr 13.76 Gyr 13.77 ± 0.13 Gyr 13.76 ± 0.11 Gyr a The parameters listed here are derived using the RECFAST 1.5 and version 4.1 of the WMAP[WMAP-7likelihood 1001.4538] code. -
FRW Type Cosmologies with Adiabatic Matter Creation
Brown-HET-991 March 1995 FRW Type Cosmologies with Adiabatic Matter Creation J. A. S. Lima1,2, A. S. M. Germano2 and L. R. W. Abramo1 1 Physics Department, Brown University, Providence, RI 02912,USA. 2 Departamento de F´ısica Te´orica e Experimental, Universidade Federal do Rio Grande do Norte, 59072 - 970, Natal, RN, Brazil. Abstract Some properties of cosmological models with matter creation are inves- tigated in the framework of the Friedman-Robertson-Walker (FRW) line element. For adiabatic matter creation, as developed by Prigogine arXiv:gr-qc/9511006v1 2 Nov 1995 and coworkers, we derive a simple expression relating the particle num- ber density n and energy density ρ which holds regardless of the mat- ter creation rate. The conditions to generate inflation are discussed and by considering the natural phenomenological matter creation rate ψ = 3βnH, where β is a pure number of the order of unity and H is the Hubble parameter, a minimally modified hot big-bang model is proposed. The dynamic properties of such models can be deduced from the standard ones simply by replacing the adiabatic index γ of the equation of state by an effective parameter γ∗ = γ(1 β). The − thermodynamic behavior is determined and it is also shown that ages large enough to agree with observations are obtained even given the high values of H suggested by recent measurements. 1 Introduction The origin of the material content (matter plus radiation) filling the presently observed universe remains one of the most fascinating unsolved mysteries in cosmology even though many authors worked out to understand the matter creation process and its effects on the evolution of the universe [1-27]. -
Universe Model Multicomponent
We can’t solve problems by using the same kind of thinking we used when we created them. Albert Einstein WORLD – UNIVERSE MODEL MULTICOMPONENT DARK MATTER COSMIC GAMMA-RAY BACKGROUND Vladimir S. Netchitailo Biolase Inc., 4 Cromwell, Irvine CA 92618, USA. [email protected] ABSTRACT World – Universe Model is based on two fundamental parameters in various rational exponents: Fine-structure constant α, and dimensionless quantity Q. While α is constant, Q increases with time, and is in fact a measure of the size and the age of the World. The Model makes predictions pertaining to masses of dark matter (DM) particles and explains the diffuse cosmic gamma-ray background radiation as the sum of contributions of multicomponent self-interacting dark matter annihilation. The signatures of DM particles annihilation with predicted masses of 1.3 TeV, 9.6 GeV, 70 MeV, 340 keV, and 3.7 keV, which are calculated independently of astrophysical uncertainties, are found in spectra of the diffuse gamma-ray background and the emission of various macroobjects in the World. The correlation between different emission lines in spectra of macroobjects is connected to their structure, which depends on the composition of the core and surrounding shells made up of DM particles. Thus the diversity of Very High Energy (VHE) gamma-ray sources in the World has a clear explanation. 1 1. INTRODUCTION In 1937, Paul Dirac proposed a new basis for cosmology: the hypothesis of a time varying gravitational “constant” [1]. In 1974, Dirac added a mechanism of continuous creation of matter in the World [2]: One might assume that nucleons are created uniformly throughout space, and thus mainly in intergalactic space. -
Galaxy Formation Within the Classical Big Bang Cosmology
Galaxy formation within the classical Big Bang Cosmology Bernd Vollmer CDS, Observatoire astronomique de Strasbourg Outline • some basics of astronomy small structure • galaxies, AGNs, and quasars • from galaxies to the large scale structure of the universe large • the theory of cosmology structure • measuring cosmological parameters • structure formation • galaxy formation in the cosmological framework • open questions small structure The architecture of the universe • Earth (~10-9 ly) • solar system (~6 10-4 ly) • nearby stars (> 5 ly) • Milky Way (~6 104 ly) • Galaxies (>2 106 ly) • large scale structure (> 50 106 ly) How can we investigate the universe Astronomical objects emit elctromagnetic waves which we can use to study them. BUT The earth’s atmosphere blocks a part of the electromagnetic spectrum. need for satellites Back body radiation • Opaque isolated body at a constant temperature Wien’s law: sun/star (5500 K): 0.5 µm visible human being (310 K): 9 µm infrared molecular cloud (15 K): 200 µm radio The structure of an atom Components: nucleus (protons, neutrons) + electrons Bohr’s model: the electrons orbit around the nucleus, the orbits are discrete Bohr’s model is too simplistic quantum mechanical description The emission of an astronomical object has 2 components: (i) continuum emission + (ii) line emission Stellar spectra Observing in colors Usage of filters (Johnson): U (UV), B (blue), V (visible), R (red), I (infrared) The Doppler effect • Is the apparent change in frequency and wavelength of a wave which is emitted by -
Searches for Leptophilic Dark Matter with Astrophysical Experiments
. Searches for leptophilic dark matter with astrophysical experiments . Von der Fakult¨atf¨urMathematik, Informatik und Naturwissenschaften der RWTH Aachen University zur Erlangung des akademischen Grades einer Doktorin der Naturwissenschaften genehmigte Dissertation vorgelegt von M. Sc. Leila Ali Cavasonza aus Finale Ligure, Savona, Italien Berichter: Universit¨atsprofessorDr. rer. nat. Michael Kr¨amer Universit¨atsprofessorDr. rer. nat. Stefan Schael Tag der m¨undlichen Pr¨ufung: 13.05.16 Diese Dissertation ist auf den Internetseiten der Universit¨atsbibliothekonline verf¨ugbar RWTH Aachen University Leila Ali Cavasonza Institut f¨urTheoretische Teilchenphysik und Kosmologie Searches for leptophilic dark matter with astrophysical experiments PhD Thesis February 2016 Supervisors: Prof. Dr. Michael Kr¨amer Prof. Dr. Stefan Schael Zusammenfassung Suche nach leptophilischer dunkler Materie mit astrophysikalischen Experimenten Die Natur der dunklen Materie (DM) zu verstehen ist eines der wichtigsten Ziele der Teilchen- und Astroteilchenphysik. Große experimentelle Anstrengungen werden un- ternommen, um die dunkle Materie nachzuweisen, in der Annahme, dass sie neben der Gravitationswechselwirkung eine weitere Wechselwirkung mit gew¨ohnlicher Materie hat. Die dunkle Materie in unserer Galaxie k¨onnte gew¨ohnliche Teilchen durch An- nihilationsprozesse erzeugen und der kosmischen Strahlung einen zus¨atzlichen Beitrag hinzuf¨ugen.Deswegen sind pr¨aziseMessungen der Fl¨ussekosmischer Strahlung ¨außerst wichtig. Das AMS-02 Experiment misst die -
FRW Cosmology
17/11/2016 Cosmology 13.8 Gyrs of Big Bang History Gravity Ruler of the Universe 1 17/11/2016 Strong Nuclear Force Responsible for holding particles together inside the nucleus. The nuclear strong force carrier particle is called the gluon. The nuclear strong interaction has a range of 10‐15 m (diameter of a proton). Electromagnetic Force Responsible for electric and magnetic interactions, and determines structure of atoms and molecules. The electromagnetic force carrier particle is the photon (quantum of light) The electromagnetic interaction range is infinite. Weak Force Responsible for (beta) radioactivity. The weak force carrier particles are called weak gauge bosons (Z,W+,W‐). The nuclear weak interaction has a range of 10‐17 m (1% of proton diameter). Gravity Responsible for the attraction between masses. Although the gravitational force carrier The hypothetical (carrier) particle is the graviton. The gravitational interaction range is infinite. By far the weakest force of nature. 2 17/11/2016 The weakest force, by far, rules the Universe … Gravity has dominated its evolution, and determines its fate … Grand Unified Theories (GUT) Grand Unified Theories * describe how ∑ Strong ∑ Weak ∑ Electromagnetic Forces are manifestations of the same underlying GUT force … * This implies the strength of the forces to diverge from their uniform GUT strength * Interesting to see whether gravity at some very early instant unifies with these forces ??? 3 17/11/2016 Newton’s Static Universe ∑ In two thousand years of astronomy, no one ever guessed that the universe might be expanding. ∑ To ancient Greek astronomers and philosophers, the universe was seen as the embodiment of perfection, the heavens were truly heavenly: – unchanging, permanent, and geometrically perfect. -
“De Sitter Effect” in the Rise of Modern Relativistic Cosmology
The role played by the “de Sitter effect” in the rise of modern relativistic cosmology ● Matteo Realdi ● Department of Astronomy, Padova ● Sait 2009. Pisa, 7-5-2009 Table of contents ● Introduction ● 1917: Einstein, de Sitter and the universes of General Relativity ● 1920's: the debates on the “de Sitter effect”. The connection between theory and observation and the rise of scientific cosmology ● 1930: the expanding universe and the decline of the interest in the de Sitter effect ● Conclusion 1 - Introduction ● Modern cosmology: study of the origin, structure and evolution of the universe as a whole, based on the interpretation of astronomical observations at different wave- lengths through the laws of physics ● The early years: 1917-1930. Extremely relevant period, characterized by new ideas, discoveries, controversies, in the light of the first comparison of theoretical world-models with observations at the turning point of relativity revolution ● Particular attention on the interest in the so-called “de Sitter effect”, a theoretical redshift-distance relation which is predicted through the line element of the empty universe of de Sitter ● The de Sitter effect: fundamental influence in contributions that scientists as de Sitter, Eddington, Weyl, Lanczos, Lemaître, Robertson, Tolman, Silberstein, Wirtz, Lundmark, Stromberg, Hubble offered during the 1920's both in theoretical and in observational cosmology (emergence of the modern approach of cosmologists) ➔ Predictions and confirmations of an appropriate redshift- distance relation marked the tortuous process towards the change of viewpoint from the 1917 paradigm of a static universe to the 1930 picture of an expanding universe evolving both in space and in time 2 - 1917: the Universes of General Relativity ● General relativity: a suitable theory in order to describe the whole of space, time and gravitation? ● Two different metrics, i.e. -
AST4220: Cosmology I
AST4220: Cosmology I Øystein Elgarøy 2 Contents 1 Cosmological models 1 1.1 Special relativity: space and time as a unity . 1 1.2 Curvedspacetime......................... 3 1.3 Curved spaces: the surface of a sphere . 4 1.4 The Robertson-Walker line element . 6 1.5 Redshifts and cosmological distances . 9 1.5.1 Thecosmicredshift . 9 1.5.2 Properdistance. 11 1.5.3 The luminosity distance . 13 1.5.4 The angular diameter distance . 14 1.5.5 The comoving coordinate r ............... 15 1.6 TheFriedmannequations . 15 1.6.1 Timetomemorize! . 20 1.7 Equationsofstate ........................ 21 1.7.1 Dust: non-relativistic matter . 21 1.7.2 Radiation: relativistic matter . 22 1.8 The evolution of the energy density . 22 1.9 The cosmological constant . 24 1.10 Some classic cosmological models . 26 1.10.1 Spatially flat, dust- or radiation-only models . 27 1.10.2 Spatially flat, empty universe with a cosmological con- stant............................ 29 1.10.3 Open and closed dust models with no cosmological constant.......................... 31 1.10.4 Models with more than one component . 34 1.10.5 Models with matter and radiation . 35 1.10.6 TheflatΛCDMmodel. 37 1.10.7 Models with matter, curvature and a cosmological con- stant............................ 40 1.11Horizons.............................. 42 1.11.1 Theeventhorizon . 44 1.11.2 Theparticlehorizon . 45 1.11.3 Examples ......................... 46 I II CONTENTS 1.12 The Steady State model . 48 1.13 Some observable quantities and how to calculate them . 50 1.14 Closingcomments . 52 1.15Exercises ............................. 53 2 The early, hot universe 61 2.1 Radiation temperature in the early universe .