The Philosopher of the Big Bounce
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Cosmic Questions, Answers Pending
special section | cosmic questions, Answers pending Cosmic questions, answers pending throughout human history, great missions of mission reveal the exploration have been inspired by curiosity, : the desire to find out about unknown realms. secrets of the universe such missions have taken explorers across wide oceans and far below their surfaces, THE OBJECTIVE deep into jungles, high onto mountain peaks For millennia, people have turned to the heavens in search of clues to nature’s mysteries. truth seekers from ages past to the present day and over vast stretches of ice to the earth’s have found that the earth is not the center of the universe, that polar extremities. countless galaxies dot the abyss of space, that an unknown form of today’s greatest exploratory mission is no matter and dark forces are at work in shaping the cosmos. Yet despite longer earthbound. it’s the scientific quest to these heroic efforts, big cosmological questions remain unresolved: explain the cosmos, to answer the grandest What happened before the Big Bang? ............................... Page 22 questions about the universe as a whole. What is the universe made of? ......................................... Page 24 what is the identity, for example, of the Is there a theory of everything? ....................................... Page 26 Are space and time fundamental? .................................... Page 28 “dark” ingredients in the cosmic recipe, com- What is the fate of the universe? ..................................... Page 30 posing 95 percent of the -
Big Bang Blunder Bursts the Multiverse Bubble
WORLD VIEW A personal take on events IER P P. PA P. Big Bang blunder bursts the multiverse bubble Premature hype over gravitational waves highlights gaping holes in models for the origins and evolution of the Universe, argues Paul Steinhardt. hen a team of cosmologists announced at a press world will be paying close attention. This time, acceptance will require conference in March that they had detected gravitational measurements over a range of frequencies to discriminate from fore- waves generated in the first instants after the Big Bang, the ground effects, as well as tests to rule out other sources of confusion. And Worigins of the Universe were once again major news. The reported this time, the announcements should be made after submission to jour- discovery created a worldwide sensation in the scientific community, nals and vetting by expert referees. If there must be a press conference, the media and the public at large (see Nature 507, 281–283; 2014). hopefully the scientific community and the media will demand that it According to the team at the BICEP2 South Pole telescope, the is accompanied by a complete set of documents, including details of the detection is at the 5–7 sigma level, so there is less than one chance systematic analysis and sufficient data to enable objective verification. in two million of it being a random occurrence. The results were The BICEP2 incident has also revealed a truth about inflationary the- hailed as proof of the Big Bang inflationary theory and its progeny, ory. The common view is that it is a highly predictive theory. -
Analysis of Big Bounce in Einstein--Cartan Cosmology
Analysis of big bounce in Einstein{Cartan cosmology Jordan L. Cubero∗ and Nikodem J. Poplawski y Department of Mathematics and Physics, University of New Haven, 300 Boston Post Road, West Haven, CT 06516, USA We analyze the dynamics of a homogeneous and isotropic universe in the Einstein{Cartan theory of gravity. The spin of fermions produces spacetime torsion that prevents gravitational singularities and replaces the big bang with a nonsingular big bounce. We show that a closed universe exists only when a particular function of its scale factor and temperature is higher than some threshold value, whereas an open and a flat universes do not have such a restriction. We also show that a bounce of the scale factor is double: as the temperature increases and then decreases, the scale factor decreases, increases, decreases, and then increases. Introduction. The Einstein{Cartan (EC) theory of a size where the cosmological constant starts cosmic ac- gravity provides the simplest mechanism generating a celeration. This expansion also predicts the cosmic mi- nonsingular big bounce, without unknown parameters crowave background radiation parameters that are con- or hypothetical fields [1]. EC is the simplest and most sistent with the Planck 2015 observations [11], as was natural theory of gravity with torsion, in which the La- shown in [12]. grangian density for the gravitational field is proportional The spin-fluid description of matter is the particle ap- to the Ricci scalar, as in general relativity [2, 3]. The con- proximation of the multipole expansion of the integrated sistency of the conservation law for the total (orbital plus conservation laws in EC. -
The Anthropic Principle and Multiple Universe Hypotheses Oren Kreps
The Anthropic Principle and Multiple Universe Hypotheses Oren Kreps Contents Abstract ........................................................................................................................................... 1 Introduction ..................................................................................................................................... 1 Section 1: The Fine-Tuning Argument and the Anthropic Principle .............................................. 3 The Improbability of a Life-Sustaining Universe ....................................................................... 3 Does God Explain Fine-Tuning? ................................................................................................ 4 The Anthropic Principle .............................................................................................................. 7 The Multiverse Premise ............................................................................................................ 10 Three Classes of Coincidence ................................................................................................... 13 Can The Existence of Sapient Life Justify the Multiverse? ...................................................... 16 How unlikely is fine-tuning? .................................................................................................... 17 Section 2: Multiverse Theories ..................................................................................................... 18 Many universes or all possible -
White-Hole Dark Matter and the Origin of Past Low-Entropy Francesca Vidotto, Carlo Rovelli
White-hole dark matter and the origin of past low-entropy Francesca Vidotto, Carlo Rovelli To cite this version: Francesca Vidotto, Carlo Rovelli. White-hole dark matter and the origin of past low-entropy. 2018. hal-01771746 HAL Id: hal-01771746 https://hal.archives-ouvertes.fr/hal-01771746 Preprint submitted on 20 Apr 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 White-hole dark matter and the origin of past low-entropy Francesca Vidotto University of the Basque Country UPV/EHU, Departamento de F´ısicaTe´orica,Barrio Sarriena, 48940 Leioa, Spain [email protected] Carlo Rovelli CPT, Aix-Marseille Universit´e,Universit´ede Toulon, CNRS, case 907, Campus de Luminy, 13288 Marseille, France [email protected] Submission date April 1, 2018 Abstract Recent results on the end of black hole evaporation give new weight to the hypothesis that a component of dark matter could be formed by remnants of evaporated black holes: stable Planck-size white holes with a large interior. The expected lifetime of these objects is consistent with their production at reheating. But remnants could also be pre-big bang relics in a bounce cosmology, and this possibility has strong implications on the issue of the source of past low entropy: it could realise a perspectival interpretation of past low entropy. -
Pushing the Limits of Time Beyond the Big Bang Singularity: Scenarios for the Branch Cut Universe
Received 05 april 2021; Revised 11 april 2021; Accepted 17 april 2021 DOI: xxx/xxxx ARTICLE TYPE Pushing the limits of time beyond the Big Bang singularity: Scenarios for the branch cut universe César A. Zen Vasconcellos*1,2 | Peter O. Hess3,4 | Dimiter Hadjimichef1 | Benno Bodmann5 | Moisés Razeira6 | Guilherme L. Volkmer1 1Instituto de Física, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre, Brazil In this contribution we identify two scenarios for the evolutionary branch cut uni- 2International Center for Relativistic verse. In the first scenario, the universe evolves continuously from the negative Astrophysics Network (ICRANet), Pescara, Italy complex cosmological time sector, prior to a primordial singularity, to the positive 3Universidad Nacional Autónoma de one, circumventing continuously a branch cut, and no primordial singularity occurs Mexico (UNAM), México City, México in the imaginary sector, only branch points. In the second scenario, the branch cut 4Frankfurt Institute for Advanced Studies (FIAS), J.W. von Goethe University and branch point disappear after the realisation of the imaginary component of the (JWGU), Hessen, Germany complex time by means of a Wick rotation, which is replaced by the thermal time. In 5 Unversidade Federal de Santa Maria the second scenario, the universe has its origin in the Big Bang, but the model con- (UFSM), Santa Maria, Brazil 6Laboratório de Geociências Espaciais e templates simultaneously a mirrored parallel evolutionary universe going backwards Astrofísica (LaGEA), Universidade Federal in the cosmological thermal time negative sector. A quantum formulation based on do PAMPA (UNIPAMPA), Caçapava do the WDW equation is sketched and preliminary conclusions are drawn. -
A Physico-Chemical Approach to Understanding Cosmic Evolution: Thermodynamics of Expansion and Composition of the Universe
A Physico-Chemical Approach To Understanding Cosmic Evolution: Thermodynamics Of Expansion And Composition Of The Universe Carlos A. Melendres ( [email protected] ) The SHD Institute Research Article Keywords: Physical and Astrochemistry, composition and expansion of the universe, thermodynamics, phase diagram, Quantum Space, spaceons, dark energy, dark matter, cosmological constant, cosmic uid, Quintessence Posted Date: March 17th, 2021 DOI: https://doi.org/10.21203/rs.3.rs-306782/v1 License: This work is licensed under a Creative Commons Attribution 4.0 International License. Read Full License A PHYSICO-CHEMICAL APPROACH TO UNDERSTANDING COSMIC EVOLUTION: THERMODYNAMICS OF EXPANSION AND COMPOSITION OF THE UNIVERSE Carlos A. Melendres The SHD Institute 216 F Street, Davis, CA 95616, U.S.A. Email: [email protected] February 2021 (Prepared for: SCIENTIFIC REPORTS) Keywords: Physical and Astrochemistry, composition and expansion of the universe, thermodynamics, phase diagram, Quantum Space, spaceons, dark energy, dark matter, cosmological constant, cosmic fluid, Quintessence 1 A PHYSICO-CHEMICAL APPROACH TO UNDERSTANDING COSMIC EVOLUTION: THERMODYNAMICS OF EXPANSION AND COMPOSITION OF THE UNIVERSE Carlos A. Melendres [email protected] ABSTRACT We present a physico-chemical approach towards understanding the mysteries associated with the Inflationary Big Bang model of Cosmic evolution, based on a theory that space consists of energy quanta. We use thermodynamics to elucidate the expansion of the universe, its composition, and the nature of dark energy and dark matter. The universe started from an atomic size volume of space quanta at very high temperature. Upon expansion and cooling, phase transitions resulted in the formation of fundamental particles, and matter which grow into stars, galaxies, and clusters due to gravity. -
Explanation of Time Travel Using Big Bounce
Explanation of time travel using big bounce Sarvesh Gharat, Btech Entc, VIIT Pune Email:- sarvesh. [email protected] Abstract:-We are going to see a short description on what exactly big bounce theory is and also we know that as per most of the theories, we know that time is nothing but just a 4th dimension.So there are many questions and paradoxes which occur if we talk about a thing called time travel. But today we are going to provide a solution for twin paradox and also are going to see, whether we can move into past, if yes then in which condition we will move into past i.e any year and in which condition we will move into past with respect to time moving in future i.e past wrt normal frame of reference but limited to the year in which we started traveling. Keywords:- Time dilation, M theory , universe, big bounce , expansion of universe , dimension, time Introduction:-There are many theories regarding formation of our universe, but one of the most accepted theory till now is the big bounce theory which says that our universe is expanding for now and will contract after some billion of years. We also know that as per M theory there are 11 dimensions out of which time is the 4th dimension. So in this paper we are going to explain how does time dilation works with the help of expansion of our universe and also what will happen to time when universe will start to contradict as mentioned in later part of big bounce theory Big bounce theory:- We all are aware of the big bounce theory which is been applied to our universe. -
DESY Workshop Combines Gravity and Particle Physics
DESY WORKSHOP DESY workshop combines gravity and particle physics Gravity and particle physics took centre stage at last year's DESY theory workshop. As chairman of the organizing committee Dieter Liist reports, there was plenty to talk about. The relationship between astro the basic ingredients of the physics, cosmology and elemen Standard Model. tary particle physics is fruitful •The choice of topics - gravity and has been constantly evolv and particle physics - for the ing for many years. Important 2001 DESY workshop (held in puzzles in cosmology can find Hamburg) was largely influ their natural explanation in enced by impressive recent microscopic particle physics, astrophysical observations and a discovery in astrophysics showing that the overall mass can sometimes give new and energy density of today's insights into the structure of universe is extremely close to its fundamental interactions. The critical value (Q = 1). Another inflationary universe scenario main theme of the workshop offers a good example. Inflation was string theories, particularly is a beautiful way to understand Wilfhed Buchmulier of DESY (left) in discussion with Hans-Peter the recently developed M-theory the cosmological flatness and Nilles of Bonn University at the DESY theory workshop. (often dubbed "the mother of all horizon problems (see box over theories") that underlies string leaf) and apparently induces large-scale density fluctuations con theories. In string and M-theory, multidimensional surfaces, rather sistent with experimental observations. Inflation also predicts the than just strings, are also allowed.These higher-dimensional mem existence of dark matter elementary particles together with a certain branes (or branes) and one particular type, Dirichlet, or D-branes, amount of dark energy manifested as the cosmological constant A. -
Arxiv:1307.1848V3 [Hep-Th] 8 Nov 2013 Tnadmdla O Nris N H Urn Ig Vacuum Higgs Data
Local Conformal Symmetry in Physics and Cosmology Itzhak Bars Department of Physics and Astronomy, University of Southern California, Los Angeles, CA, 90089-0484, USA, Paul Steinhardt Physics Department, Princeton University, Princeton NJ08544, USA, Neil Turok Perimeter Institute for Theoretical Physics, Waterloo, ON N2L 2Y5, Canada. (Dated: July 7, 2013) Abstract We show how to lift a generic non-scale invariant action in Einstein frame into a locally conformally-invariant (or Weyl-invariant) theory and present a new general form for Lagrangians consistent with Weyl symmetry. Advantages of such a conformally invariant formulation of particle physics and gravity include the possibility of constructing geodesically complete cosmologies. We present a conformal-invariant version of the standard model coupled to gravity, and show how Weyl symmetry may be used to obtain unprecedented analytic control over its cosmological solutions. Within this new framework, generic FRW cosmologies are geodesically complete through a series of big crunch - big bang transitions. We discuss a new scenario of cosmic evolution driven by the Higgs field in a “minimal” conformal standard model, in which there is no new physics beyond the arXiv:1307.1848v3 [hep-th] 8 Nov 2013 standard model at low energies, and the current Higgs vacuum is metastable as indicated by the latest LHC data. 1 Contents I. Why Conformal Symmetry? 3 II. Why Local Conformal Symmetry? 8 A. Global scale invariance 8 B. Local scale invariance 11 III. General Weyl Symmetric Theory 15 A. Gravity 15 B. Supergravity 22 IV. Conformal Cosmology 25 Acknowledgments 31 References 31 2 I. WHY CONFORMAL SYMMETRY? Scale invariance is a well-known symmetry [1] that has been studied in many physical contexts. -
Traversing Cosmological Singularities, Complete Journeys Through Spacetime Including Antigravity
Traversing Cosmological Singularities Complete Journeys Through Spacetime Including Antigravity ∗ Itzhak Bars Department of Physics and Astronomy, University of Southern California, Los Angeles, CA 90089-0484, USA A unique description of the Big Crunch-Big Bang transition is given at the classical gravity level, along with a complete set of homogeneous, isotropic, analytic solutions in scalar-tensor cosmology, with radiation and curvature. All solutions repeat cyclically; they have been obtained by using conformal gauge symmetry (Weyl symmetry) as a powerful tool in cosmology, and more generally in gravity. The significance of the Big Crunch-Big Bang transition is that it provides a model inde- pendent analytic resolution of the singularity, as an unambiguous and unavoidable solution of the equations at the classical gravitational physics level. It is controlled only by geometry (including anisotropy) and only very general features of matter coupled to gravity, such as kinetic energy of a scalar field, and radiation due to all forms of relativistic matter. This analytic resolution of the singularity is due to an attractor mechanism created by the leading terms in the cosmological equa- tion. It is unique, and it is unavoidable in classical relativity in a geodesically complete geometry. Its counterpart in quantum gravity remains to be understood. I. INTRODUCTION AND SUMMARY OF RESULTS Resolving the big bang singularity is one of the central challenges for fundamental physics and cosmology. The issue arises naturally in the context of classical relativity due to the geodesically incomplete nature of the singular spacetime [1]-[2]. The resolution may not be completed until the physics is understood in the context of quantum gravity. -
The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big
View metadata, citation and similar papers at core.ac.uk brought to you by CORE The Ekpyrotic Universe: Colliding Branes and the Origin ofprovided the by CERN Document Server Hot Big Bang Justin Khoury1,BurtA.Ovrut2,PaulJ.Steinhardt1 and Neil Turok 3 1 Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA 2 Department of Physics, University of Pennsylvania, Philadelphia, PA 19104-6396, USA 3 DAMTP, CMS, Wilberforce Road, Cambridge, CB3 0WA, UK Abstract We propose a cosmological scenario in which the hot big bang universe is produced by the collision of a brane in the bulk space with a bounding orb- ifold plane, beginning from an otherwise cold, vacuous, static universe. The model addresses the cosmological horizon, flatness and monopole problems and generates a nearly scale-invariant spectrum of density perturbations with- out invoking superluminal expansion (inflation). The scenario relies, instead, on physical phenomena that arise naturally in theories based on extra di- mensions and branes. As an example, we present our scenario predominantly within the context of heterotic M-theory. A prediction that distinguishes this scenario from standard inflationary cosmology is a strongly blue gravitational wave spectrum, which has consequences for microwave background polariza- tion experiments and gravitational wave detectors. Typeset using REVTEX 1 I. INTRODUCTION The Big Bang model provides an accurate account of the evolution of our universe from the time of nucleosynthesis until the present, but does not address the key