The Sun Liquid Or Gaseous?

Total Page:16

File Type:pdf, Size:1020Kb

The Sun Liquid Or Gaseous? 2011 Volume 3 The Journal on Advanced Studies in Theoretical and Experimental Physics, including Related Themes from Mathematics PROGRESS IN PHYSICS SPECIAL ISSUE The Sun — Liquid or Gaseous? A Thermodynamic Analysis “All scientists shall have the right to present their scientific research results, in whole or in part, at relevant scientific conferences, and to publish the same in printed scientific journals, electronic archives, and any other media.” — Declaration of Academic Freedom, Article 8 ISSN 1555-5534 The Journal on Advanced Studies in Theoretical and Experimental Physics, including Related Themes from Mathematics PROGRESS IN PHYSICS A quarterly issue scientific journal, registered with the Library of Congress (DC, USA). This journal is peer reviewed and included in the abs- tracting and indexing coverage of: Mathematical Reviews and MathSciNet (AMS, USA), DOAJ of Lund University (Sweden), Zentralblatt MATH (Germany), Scientific Commons of the University of St. Gallen (Switzerland), Open-J-Gate (India), Referativnyi Zhurnal VINITI (Russia), etc. Electronic version of this journal: JULY 2011 VOLUME 3 http://www.ptep-online.com Editorial Board Dmitri Rabounski, Editor-in-Chief SPECIAL ISSUE [email protected] Florentin Smarandache, Assoc. Editor [email protected] The Sun — Gaseous or Liquid? Larissa Borissova, Assoc. Editor [email protected] A Thermodynamic Analysis Editorial Team Gunn Quznetsov [email protected] Andreas Ries CONTENTS [email protected] Chifu Ebenezer Ndikilar [email protected] Robitaille P.M. A Thermodynamic History of the Solar Constitution — I: The Journey Felix Scholkmann toaGaseousSun.............................................................3 [email protected] Secchi A. On the Theory of Solar Spots Proposed by Signor Kirchoff ..................26 Postal Address Secchi A. On the Structure of the Solar Photosphere. .30 Department of Mathematics and Science, Magnus G. A Note on the Constitution of the Sun . 33 University of New Mexico, 200 College Road, Gallup, NM 87301, USA Faye H. On the Physical Constitution of the Sun — Part I. .35 Robitaille P.M. A Thermodynamic History of the Solar Constitution — II: The Theory of a Gaseous Sun and Jeans’ Failed Liquid Alternative. .41 Copyright c Progress in Physics, 2011 All rights reserved. The authors of the ar- Robitaille P.M. Liquid Metallic Hydrogen: A Building Block for the Liquid Sun . 60 ticles do hereby grant Progress in Physics Robitaille P.M. On the Presence of a Distinct Solar Surface: A Reply to Herve´ Faye . 75 non-exclusive, worldwide, royalty-free li- Robitaille P.M. On Solar Granulations, Limb Darkening, and Sunspots: Brief Insights cense to publish and distribute the articles in accordance with the Budapest Open Initia- in Remembrance of Father Angelo Secchi . 79 tive: this means that electronic copying, dis- Robitaille P.M. On the Temperature of the Photosphere: Energy Partition in the Sun . 89 tribution and printing of both full-size ver- sion of the journal and the individual pa- Robitaille P.M. Stellar Opacity: The Achilles Heel of a Gaseous Sun . 93 pers published therein for non-commercial, Robitaille P.M. LessonsfromtheSun.............................................100 academic or individual use can be made by any user without permission or charge. The LETTERS authors of the articles published in Progress in Physics retain their rights to use this jour- Dmitri Rabounski Pierre-Marie Luc Robitaille . L1 nal as a whole or any part of it in any other publications and in any way they see fit. Any part of Progress in Physics howsoever used in other publications must include an appropriate citation of this journal. This journal is powered by LATEX A variety of books can be downloaded free from the Digital Library of Science: http://www.gallup.unm.edu/ smarandache ∼ ISSN: 1555-5534 (print) ISSN: 1555-5615 (online) Standard Address Number: 297-5092 Printed in the United States of America Information for Authors and Subscribers Progress in Physics has been created for publications on advanced studies in theoretical and experimental physics, including related themes from mathe- matics and astronomy. All submitted papers should be professional, in good English, containing a brief review of a problem and obtained results. All submissions should be designed in LATEX format using Progress in Physics template. This template can be downloaded from Progress in Physics home page http://www.ptep-online.com. Abstract and the necessary informa- tion about author(s) should be included into the papers. To submit a paper, mail the file(s) to the Editor-in-Chief. All submitted papers should be as brief as possible. We accept brief pa- pers, no larger than 8 typeset journal pages. Short articles are preferable. Large papers can be considered in exceptional cases to the section Special Reports intended for such publications in the journal. Letters related to the publications in the journal or to the events among the science community can be applied to the section Letters to Progress in Physics. All that has been accepted for the online issue of Progress in Physics is printed in the paper version of the journal. To order printed issues, contact the Editors. This journal is non-commercial, academic edition. It is printed from pri- vate donations. (Look for the current author fee in the online version of the journal.) July, 2011 PROGRESS IN PHYSICS Volume 3 A Thermodynamic History of the Solar Constitution — I: The Journey to a Gaseous Sun Pierre-Marie Robitaille Department of Radiology, The Ohio State University, 395 W. 12th Ave, Suite 302, Columbus, Ohio 43210, USA E-mail: [email protected] History has the power to expose the origin and evolution of scientific ideas. How did humanity come to visualize the Sun as a gaseous plasma? Why is its interior thought to contain blackbody radiation? Who were the first people to postulate that the density of the solar body varied greatly with depth? When did mankind first conceive that the solar surface was merely an illusion? What were the foundations of such thoughts? In this regard, a detailed review of the Sun’s thermodynamic history provides both a necessary exposition of the circumstance which accompanied the acceptance of the gaseous mod- els and a sound basis for discussing modern solar theories. It also becomes an invitation to reconsider the phase of the photosphere. As such, in this work, the contributions of Pierre Simon Laplace, Alexander Wilson, William Herschel, Hermann von Helmholtz, Herbert Spencer, Richard Christopher Carrington, John Frederick William Herschel, Father Pietro Angelo Secchi, Herve´ August Etienne Albans Faye, Edward Frankland, Joseph Norman Lockyer, Warren de la Rue, Balfour Stewart, Benjamin Loewy, and Gustav Robert Kirchhoff, relative to the evolution of modern stellar models, will be discussed. Six great pillars created a gaseous Sun: 1) Laplace’s Nebular Hypothesis, 2) Helmholtz’ contraction theory of energy production, 3) Andrew’s elucidation of crit- ical temperatures, 4) Kirchhoff’s formulation of his law of thermal emission, 5) Plucker¨ and Hittorf’s discovery of pressure broadening in gases, and 6) the evolution of the stel- lar equations of state. As these are reviewed, this work will venture to highlight not only the genesis of these revolutionary ideas, but also the forces which drove great men to advance a gaseous Sun. 1 On the history of solar science ical paths followed by its founders [1–14], has at times over- Pondering upon the history of solar science [1–14], it be- looked the contributions and criticisms of “non-astronomers”. comes apparent that, in every age, the dominant theory of the Perhaps unable to accept the consequences stemming from internal constitution of the Sun reflected the state of human the discoveries of the present age, it has continued to perpet- knowledge. As understanding of the physical world grew, the uate ideas which can no longer hold any basis in the physical theories of old were slowly transformed. Eventually, under world. the burden of evidence, ancient ideas were destined to disap- 2 Pillars of a gaseous Sun pear completely from the realm of science, relinquished to the sphere of historical curiosity [2]. What was once considered Five great pillars gave birth to the gaseous Sun in the middle high thought, became discarded. and late 19th century. They were as follows: 1) Laplace’s If science is to advance, historical analysis must not solely nebular hypothesis [22, 23], 2) Helmholtz’ contraction the- reiterate the progress of civilization. Its true merit lies not in ory [24, 25], 3) Cagniard de la Tour’s discovery of critical the reminiscence of facts, the restatement of ancient ideas, phenomena [26,27] and Andrew’s elucidation of critical tem- and the reliving of time. Rather, scientific history’s virtue peratures [28, 29], 4) Kirchhoff’s formulation of his law of stems from the guidance it can impart to the evolution of mod- thermal emission [30–32], and 5) the discovery of pressure ern research. broadening in gases by Plucker,¨ Hittorf, Wullner,¨ Frankland, Historical compilations, dissected with contemporary sci- and Lockyer [33–37]. Today, the last four of these pillars entific reasoning, have the power to expose both the truths have collapsed, either as scientifically unsound (pillar 4), or and the errors which swayed our formation of a gaseous Sun as irrelevant with respect to discussions of the internal con- [15–21]. These models have evolved as a direct manifesta- stitution of the Sun and the nature of the photosphere (pillars tion of mankind’s physical knowledge in the 19th and 20th 2, 3, and 5). Only the first argument currently survives as rel- centuries. Through historical review, it can be demonstrated evant to solar theory, albeit in modified form. Nevertheless, that virtually every salient fact which endowed the Sun with each of these doctrines had acted as a driving force in creating a gaseous interior has actually been refuted or supplanted by a gaseous Sun.
Recommended publications
  • Smithsonian Miscellaneous Collections
    BULLETIN PHILOSOPHICAL SOCIETY WASHINGTON. VOL. IV. Containing the Minutes of the Society from the 185th Meeting, October 9, 1880, to the 2020! Meeting, June 11, 1881. PUBLISHED BY THE CO-OPERATION OF THE SMITHSONIAN INSTITUTION. WASHINGTON JUDD & DETWEILER, PRINTERS, WASHINGTON, D. C. CONTENTS. PAGE. Constitution of the Philosophical Society of Washington 5 Standing Rules of the Society 7 Standing Rules of the General Committee 11 Rules for the Publication of the Bulletin 13 List of Members of the Society 15 Minutes of the 185th Meeting, October 9th, 1880. —Cleveland Abbe on the Aurora Borealis , 21 Minutes of the 186th Meeting, October 25th, 1880. —Resolutions on the decease of Prof. Benj. Peirce, with remarks thereon by Messrs. Alvord, Elliott, Hilgard, Abbe, Goodfellow, and Newcomb. Lester F. Ward on the Animal Population of the Globe 23 Minutes of the 187th Meeting, November 6th, 1880. —Election of Officers of the Society. Tenth Annual Meeting 29 Minutes of the 188th Meeting, November 20th, 1880. —John Jay Knox on the Distribution of Loans in the Bank of France, the National Banks of the United States, and the Imperial of Bank Germany. J. J. Riddell's Woodward on Binocular Microscope. J. S. Billings on the Work carried on under the direction of the National Board of Health, 30 Minutes of the 189th Meeting, December 4th, 1880. —Annual Address of the retiring President, Simon Newcomb, on the Relation of Scientific Method to Social Progress. J. E. Hilgard on a Model of the Basin of the Gulf of Mexico 39 Minutes of the 190th Meeting, December iSth, 1880.
    [Show full text]
  • Small, Young Volcanic Deposits Around the Lunar Farside Craters Rosseland, Bolyai, and Roche
    44th Lunar and Planetary Science Conference (2013) 2024.pdf SMALL, YOUNG VOLCANIC DEPOSITS AROUND THE LUNAR FARSIDE CRATERS ROSSELAND, BOLYAI, AND ROCHE. J. H. Pasckert1, H. Hiesinger1, and C. H. van der Bogert1. 1Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany. jhpasckert@uni- muenster.de Introduction: To understand the thermal evolu- mare basalts on the near- and farside. This gives us the tion of the Moon it is essential to investigate the vol- opportunity to investigate the history of small scale canic history of both the lunar near- and farside. While volcanism on the lunar farside. the lunar nearside is dominated by mare volcanism, the farside shows only some isolated mare deposits in the large craters and basins, like the South Pole-Aitken basin or Tsiolkovsky crater [e.g., 1-4]. This big differ- ence in volcanic activity between the near- and farside is of crucial importance for understanding the volcanic evolution of the Moon. The extensive mare volcanism of the lunar nearside has already been studied in great detail by numerous authors [e.g., 4-8] on the basis of Lunar Orbiter and Apollo data. New high-resolution data obtained by the Lunar Reconnaissance Orbiter (LRO) and the SELENE Terrain Camera (TC) now allow us to investigate the lunar farside in great detail. Basaltic volcanism of the lunar nearside was active for almost 3 Ga, lasting from ~3.9-4.0 Ga to ~1.2 Ga before present [5]. In contrast to the nearside, most eruptions of mare deposits on the lunar farside stopped much earlier, ~3.0 Ga ago [9].
    [Show full text]
  • Homotopy Perturbation Method with Laplace Transform (LT-HPM) Is Given in “Homotopy Perturbation Method” Section
    Tripathi and Mishra SpringerPlus (2016) 5:1859 DOI 10.1186/s40064-016-3487-4 RESEARCH Open Access Homotopy perturbation method with Laplace Transform (LT‑HPM) for solving Lane–Emden type differential equations (LETDEs) Rajnee Tripathi and Hradyesh Kumar Mishra* *Correspondence: [email protected] Abstract Department In this communication, we describe the Homotopy Perturbation Method with Laplace of Mathematics, Jaypee University of Engineering Transform (LT-HPM), which is used to solve the Lane–Emden type differential equa- and Technology, Guna, MP tions. It’s very difficult to solve numerically the Lane–Emden types of the differential 473226, India equation. Here we implemented this method for two linear homogeneous, two linear nonhomogeneous, and four nonlinear homogeneous Lane–Emden type differential equations and use their appropriate comparisons with exact solutions. In the current study, some examples are better than other existing methods with their nearer results in the form of power series. The Laplace transform used to accelerate the convergence of power series and the results are shown in the tables and graphs which have good agreement with the other existing method in the literature. The results show that LT- HPM is very effective and easy to implement. Keywords: Homotopy Perturbation Method (HPM), Laplace Transform (LT), Singular Initial value problems (IVPs), Lane–Emden type equations Background Two astrophysicists, Jonathan Homer Lane and Robert had explained the Lane–Emden type differential equations. In this study, they had designed these types of differential equations, which is a dimensionless structure of Poisson’s equation for the gravitational potential of a self-gravitating, spherically symmetric, polytropic fluid and the thermal behavior of a spherical bunch of gas according to the laws of thermodynamics (Lane 1870; Richardson 1921).
    [Show full text]
  • The Language of Differential Forms
    Appendix A The Language of Differential Forms This appendix—with the only exception of Sect.A.4.2—does not contain any new physical notions with respect to the previous chapters, but has the purpose of deriving and rewriting some of the previous results using a different language: the language of the so-called differential (or exterior) forms. Thanks to this language we can rewrite all equations in a more compact form, where all tensor indices referred to the diffeomorphisms of the curved space–time are “hidden” inside the variables, with great formal simplifications and benefits (especially in the context of the variational computations). The matter of this appendix is not intended to provide a complete nor a rigorous introduction to this formalism: it should be regarded only as a first, intuitive and oper- ational approach to the calculus of differential forms (also called exterior calculus, or “Cartan calculus”). The main purpose is to quickly put the reader in the position of understanding, and also independently performing, various computations typical of a geometric model of gravity. The readers interested in a more rigorous discussion of differential forms are referred, for instance, to the book [22] of the bibliography. Let us finally notice that in this appendix we will follow the conventions introduced in Chap. 12, Sect. 12.1: latin letters a, b, c,...will denote Lorentz indices in the flat tangent space, Greek letters μ, ν, α,... tensor indices in the curved manifold. For the matter fields we will always use natural units = c = 1. Also, unless otherwise stated, in the first three Sects.
    [Show full text]
  • Inis: Terminology Charts
    IAEA-INIS-13A(Rev.0) XA0400071 INIS: TERMINOLOGY CHARTS agree INTERNATIONAL ATOMIC ENERGY AGENCY, VIENNA, AUGUST 1970 INISs TERMINOLOGY CHARTS TABLE OF CONTENTS FOREWORD ... ......... *.* 1 PREFACE 2 INTRODUCTION ... .... *a ... oo 3 LIST OF SUBJECT FIELDS REPRESENTED BY THE CHARTS ........ 5 GENERAL DESCRIPTOR INDEX ................ 9*999.9o.ooo .... 7 FOREWORD This document is one in a series of publications known as the INIS Reference Series. It is to be used in conjunction with the indexing manual 1) and the thesaurus 2) for the preparation of INIS input by national and regional centrea. The thesaurus and terminology charts in their first edition (Rev.0) were produced as the result of an agreement between the International Atomic Energy Agency (IAEA) and the European Atomic Energy Community (Euratom). Except for minor changesq the terminology and the interrela- tionships btween rms are those of the December 1969 edition of the Euratom Thesaurus 3) In all matters of subject indexing and ontrol, the IAEA followed the recommendations of Euratom for these charts. Credit and responsibility for the present version of these charts must go to Euratom. Suggestions for improvement from all interested parties. particularly those that are contributing to or utilizing the INIS magnetic-tape services are welcomed. These should be addressed to: The Thesaurus Speoialist/INIS Section Division of Scientific and Tohnioal Information International Atomic Energy Agency P.O. Box 590 A-1011 Vienna, Austria International Atomic Energy Agency Division of Sientific and Technical Information INIS Section June 1970 1) IAEA-INIS-12 (INIS: Manual for Indexing) 2) IAEA-INIS-13 (INIS: Thesaurus) 3) EURATOM Thesaurusq, Euratom Nuclear Documentation System.
    [Show full text]
  • UCSC Special Collections and Archives MS 6 Morley Baer
    UCSC Special Collections and Archives MS 6 Morley Baer Photographs - Job Number Index Description Job Number Date Thompson Lawn 1350 1946 August Peter Thatcher 1467 undated Villa Moderne, Taylor and Vial - Carmel 1645-1951 1948 Telephone Building 1843 1949 Abrego House 1866 undated Abrasive Tools - Bob Gilmore 2014, 2015 1950 Inn at Del Monte, J.C. Warnecke. Mark Thomas 2579 1955 Adachi Florists 2834 1957 Becks - interiors 2874 1961 Nicholas Ten Broek 2878 1961 Portraits 1573 circa 1945-1960 Portraits 1517 circa 1945-1960 Portraits 1573 circa 1945-1960 Portraits 1581 circa 1945-1960 Portraits 1873 circa 1945-1960 Portraits unnumbered circa 1945-1960 [Naval Radio Training School, Monterey] unnumbered circa 1945-1950 [Men in Hardhats - Sign reads, "Hitler Asked for It! Free Labor is Building the Reply"] unnumbered circa 1945-1950 CZ [Crown Zellerbach] Building - Sonoma 81510 1959 May C.Z. - SOM 81552 1959 September C.Z. - SOM 81561 1959 September Crown Zellerbach Bldg. 81680 1960 California and Chicago: landscapes and urban scenes unnumbered circa 1945-1960 Spain 85343 1957-1958 Fleurville, France 85344 1957 Berardi fountain & water clock, Rome 85347 1980 Conciliazione fountain, Rome 84154 1980 Ferraioli fountain, Rome 84158 1980 La Galea fountain, in Vatican, Rome 84160 1980 Leone de Vaticano fountain (RR station), Rome 84163 1980 Mascherone in Vaticano fountain, Rome 84167 1980 Pantheon fountain, Rome 84179 1980 1 UCSC Special Collections and Archives MS 6 Morley Baer Photographs - Job Number Index Quatre Fountain, Rome 84186 1980 Torlonai
    [Show full text]
  • A Chronological History of Electrical Development from 600 B.C
    From the collection of the n z m o PreTinger JJibrary San Francisco, California 2006 / A CHRONOLOGICAL HISTORY OF ELECTRICAL DEVELOPMENT FROM 600 B.C. PRICE $2.00 NATIONAL ELECTRICAL MANUFACTURERS ASSOCIATION 155 EAST 44th STREET NEW YORK 17, N. Y. Copyright 1946 National Electrical Manufacturers Association Printed in U. S. A. Excerpts from this book may be used without permission PREFACE presenting this Electrical Chronology, the National Elec- JNtrical Manufacturers Association, which has undertaken its compilation, has exercised all possible care in obtaining the data included. Basic sources of information have been search- ed; where possible, those in a position to know have been con- sulted; the works of others, who had a part in developments referred to in this Chronology, and who are now deceased, have been examined. There may be some discrepancies as to dates and data because it has been impossible to obtain unchallenged record of the per- son to whom should go the credit. In cases where there are several claimants every effort has been made to list all of them. The National Electrical Manufacturers Association accepts no responsibility as being a party to supporting the claims of any person, persons or organizations who may disagree with any of the dates, data or any other information forming a part of the Chronology, and leaves it to the reader to decide for him- self on those matters which may be controversial. No compilation of this kind is ever entirely complete or final and is always subject to revisions and additions. It should be understood that the Chronology consists only of basic data from which have stemmed many other electrical developments and uses.
    [Show full text]
  • An Interpretation of Milne Cosmology
    An Interpretation of Milne Cosmology Alasdair Macleod University of the Highlands and Islands Lews Castle College Stornoway Isle of Lewis HS2 0XR UK [email protected] Abstract The cosmological concordance model is consistent with all available observational data, including the apparent distance and redshift relationship for distant supernovae, but it is curious how the Milne cosmological model is able to make predictions that are similar to this preferred General Relativistic model. Milne’s cosmological model is based solely on Special Relativity and presumes a completely incompatible redshift mechanism; how then can the predictions be even remotely close to observational data? The puzzle is usually resolved by subsuming the Milne Cosmological model into General Relativistic cosmology as the special case of an empty Universe. This explanation may have to be reassessed with the finding that spacetime is approximately flat because of inflation, whereupon the projection of cosmological events onto the observer’s Minkowski spacetime must always be kinematically consistent with Special Relativity, although the specific dynamics of the underlying General Relativistic model can give rise to virtual forces in order to maintain consistency between the observation and model frames. I. INTRODUCTION argument is that a clear distinction must be made between models, which purport to explain structure and causes (the Edwin Hubble’s discovery in the 1920’s that light from extra- ‘Why?’), and observational frames which simply impart galactic nebulae is redshifted in linear proportion to apparent consistency and causality on observation (the ‘How?’). distance was quickly associated with General Relativity (GR), and explained by the model of a closed finite Universe curved However, it can also be argued this approach does not actually under its own gravity and expanding at a rate constrained by the explain the similarity in the predictive power of Milne enclosed mass.
    [Show full text]
  • Resolving Hubble Tension with the Milne Model 3
    Resolving Hubble tension with the Milne model* Ram Gopal Vishwakarma Unidad Acade´mica de Matema´ticas Universidad Auto´noma de Zacatecas, Zacatecas C. P. 98068, ZAC, Mexico [email protected] Abstract The recent measurements of the Hubble constant based on the standard ΛCDM cos- mology reveal an underlying disagreement between the early-Universe estimates and the late-time measurements. Moreover, as these measurements improve, the discrepancy not only persists but becomes even more significant and harder to ignore. The present situ- ation places the standard cosmology in jeopardy and provides a tantalizing hint that the problem results from some new physics beyond the ΛCDM model. It is shown that a non-conventional theory - the Milne model - which introduces a different evolution dynamics for the Universe, alleviates the Hubble tension significantly. Moreover, the model also averts some long-standing problems of the standard cosmology, for instance, the problems related with the cosmological constant, the horizon, the flat- ness, the Big Bang singularity, the age of the Universe and the non-conservation of energy. Keywords: Milne model; ΛCDM model; Hubble tension; SNe Ia observations; CMB observations. arXiv:2011.12146v1 [physics.gen-ph] 20 Nov 2020 1 Introduction The Hubble constant H0 is one of the most important parameters in cosmology which mea- sures the present rate of expansion of the Universe, and thereby estimates its size and age. This is done by assuming a cosmological model. However, the two values of H0 predicted by the standard ΛCDM model, one inferred from the measurements of the early Universe and the other from the late-time local measurements, seem to be in sever tension.
    [Show full text]
  • Binary Asteroids and the Formation of Doublet Craters
    ICARUS 124, 372±391 (1996) ARTICLE NO. 0215 Binary Asteroids and the Formation of Doublet Craters WILLIAM F. BOTTKE,JR. Division of Geological and Planetary Sciences, California Institute of Technology, Mail Code 170-25, Pasadena, California 91125 E-mail: [email protected] AND H. JAY MELOSH Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721 Received April 29, 1996; revised August 14, 1996 found we could duplicate the observed fraction of doublet cra- At least 10% (3 out of 28) of the largest known impact craters ters found on Earth, Venus, and Mars. Our results suggest on Earth and a similar fraction of all impact structures on that any search for asteroid satellites should place emphasis Venus are doublets (i.e., have a companion crater nearby), on km-sized Earth-crossing asteroids with short-rotation formed by the nearly simultaneous impact of objects of compa- periods. 1996 Academic Press, Inc. rable size. Mars also has doublet craters, though the fraction found there is smaller (2%). These craters are too large and too far separated to have been formed by the tidal disruption 1. INTRODUCTION of an asteroid prior to impact, or from asteroid fragments dispersed by aerodynamic forces during entry. We propose that Two commonly held paradigms about asteroids and some fast rotating rubble-pile asteroids (e.g., 4769 Castalia), comets are that (a) they are composed of non-fragmented after experiencing a close approach with a planet, undergo tidal chunks of rock or rock/ice mixtures, and (b) they are soli- breakup and split into multiple co-orbiting fragments.
    [Show full text]
  • Structure Formation in a Dirac-Milne Universe: Comparison with the Standard Cosmological Model Giovanni Manfredi, Jean-Louis Rouet, Bruce N
    Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model Giovanni Manfredi, Jean-Louis Rouet, Bruce N. Miller, Gabriel Chardin To cite this version: Giovanni Manfredi, Jean-Louis Rouet, Bruce N. Miller, Gabriel Chardin. Structure formation in a Dirac-Milne universe: comparison with the standard cosmological model. Physical Review D, Ameri- can Physical Society, 2020, 102 (10), pp.103518. 10.1103/PhysRevD.102.103518. hal-02999626 HAL Id: hal-02999626 https://hal.archives-ouvertes.fr/hal-02999626 Submitted on 28 Jun 2021 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. Copyright PHYSICAL REVIEW D 102, 103518 (2020) Structure formation in a Dirac-Milne universe: Comparison with the standard cosmological model Giovanni Manfredi * Universit´e de Strasbourg, CNRS, Institut de Physique et Chimie des Mat´eriaux de Strasbourg, UMR 7504, F-67000 Strasbourg, France Jean-Louis Rouet Universit´ed’Orl´eans, CNRS/INSU, BRGM, ISTO, UMR7327, F-45071 Orl´eans, France Bruce N. Miller Department of Physics and Astronomy, Texas Christian University, Fort Worth, Texas 76129, USA † Gabriel Chardin Universit´e de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France (Received 15 July 2020; accepted 12 October 2020; published 13 November 2020) The presence of complex hierarchical gravitational structures is one of the main features of the observed universe.
    [Show full text]
  • Phd Projects at the Institute of Origins
    PhD projects at the Institute of Origins. A list of possible PhD projects at the Institute of Origins appear in the following pages. If you have any questions regarding any projects please contact the individual supervisors. Also if you have other suggestions for a project please contact us as well. The chemical composition of star forming regions near and far .................................... 3 ! Modelling the solubilities of organic solids in hydrocarbon liquids: application to the geology and astrobiology of Titan. .................................................................................... 4! Modeling turbulent flows in solar quiescent prominences ...............................................5! The zoo of exo-planets..................................................................................................8! Understanding the formation of heavy negative ions at Titan and Enceladus................9! Mapping anthropogenic versus natural sources of atmospheric CO2 ............................11! Probing Large Scale Structure with High Energy Neutrinos.........................................13! Future Moon Missions and High Energy Neutrinos ......................................................15! Measuring Cosmic Particles and the Upper Atmosphere with LOFAR.........................17! Mimicking planetary environments for assessing the survivability of bacterial organisms within an artificial environmental chamber. A combined planetary atmosphere and microbiological study for exploring panspermia................................
    [Show full text]