Modified Einsteinian Dynamics
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Particle Dark Matter an Introduction Into Evidence, Models, and Direct Searches
Particle Dark Matter An Introduction into Evidence, Models, and Direct Searches Lecture for ESIPAP 2016 European School of Instrumentation in Particle & Astroparticle Physics Archamps Technopole XENON1T January 25th, 2016 Uwe Oberlack Institute of Physics & PRISMA Cluster of Excellence Johannes Gutenberg University Mainz http://xenon.physik.uni-mainz.de Outline ● Evidence for Dark Matter: ▸ The Problem of Missing Mass ▸ In galaxies ▸ In galaxy clusters ▸ In the universe as a whole ● DM Candidates: ▸ The DM particle zoo ▸ WIMPs ● DM Direct Searches: ▸ Detection principle, physics inputs ▸ Example experiments & results ▸ Outlook Uwe Oberlack ESIPAP 2016 2 Types of Evidences for Dark Matter ● Kinematic studies use luminous astrophysical objects to probe the gravitational potential of a massive environment, e.g.: ▸ Stars or gas clouds probing the gravitational potential of galaxies ▸ Galaxies or intergalactic gas probing the gravitational potential of galaxy clusters ● Gravitational lensing is an independent way to measure the total mass (profle) of a foreground object using the light of background sources (galaxies, active galactic nuclei). ● Comparison of mass profles with observed luminosity profles lead to a problem of missing mass, usually interpreted as evidence for Dark Matter. ● Measuring the geometry (curvature) of the universe, indicates a ”fat” universe with close to critical density. Comparison with luminous mass: → a major accounting problem! Including observations of the expansion history lead to the Standard Model of Cosmology: accounting defcit solved by ~68% Dark Energy, ~27% Dark Matter and <5% “regular” (baryonic) matter. ● Other lines of evidence probe properties of matter under the infuence of gravity: ▸ the equation of state of oscillating matter as observed through fuctuations of the Cosmic Microwave Background (acoustic peaks). -
A Critique of Covariant Emergent Gravity
Prepared for submission to JCAP A Critique of Covariant Emergent Gravity Kirill Zatrimaylov Scuola Normale Superiore and I.N.F.N. Piazza dei Cavalieri 7, 56126, Pisa, Italy E-mail: [email protected] Abstract. I address some problems encountered in the formulation of relativistic models encompassing the MOND phenomenology of radial acceleration. I explore scalar and vector theories with fractional kinetic terms and f(R)-type gravity, demanding that the energy density be bounded from below and that superluminal modes be absent, but also that some consistency constraints with observational results hold. I identify configurations whose energy is unbounded from below and formulate some no-go statements for vector field models and arXiv:2003.10410v1 [gr-qc] 23 Mar 2020 modified gravity theories. Finally, I discuss superfluid dark matter as a hybrid theory lying between CDM and modified gravity, highlighting some difficulties present also in this case, which appears preferable to the others. Contents 1 Introduction1 2 A Brief Overview of MOND3 3 Covariant Theories with Fractional Kinetic Terms6 3.1 Scalar 8 3.2 Vector 9 3.3 Tensor 15 4 Fractional Kinetic Terms from Spontaneous Symmetry Breaking 19 5 Conclusions 20 1 Introduction MOND (Modified Newtonian dynamics), proposed by M. Milgrom in 1981 [1], was meant originally as an alternative to the cold dark matter paradigm: it aims to explain phenomena usually attributed to dark matter via Newtonian laws (either the law of gravity or the law of inertia) that are modified at large distances and small accelerations. Until recently, its actual significance has been somewhat obscure, since it does account for one class of observations (galaxy rotation curves) without addressing other key issues (CMB, primordial structure formation, and displacement between luminous and dark matter components in galaxy cluster collisions). -
X-Ray Shapes of Elliptical Galaxies and Implications for Self-Interacting Dark Matter
Prepared for submission to JCAP X-Ray Shapes of Elliptical Galaxies and Implications for Self-Interacting Dark Matter A. McDaniel,a;bc;1 T., Jeltema,b;c S., Profumob;c aDepartment of Physics and Astronomy, Kinard Lab of Physics, Clemson, SC, 29634-0978, USA bDepartment of Physics, University of California, 1156 High Street, Santa Cruz, California, 95064, USA cSanta Cruz Institute for Particle Physics, 1156 High Street, Santa Cruz, California, 95064, USA E-mail: [email protected], [email protected], [email protected] Abstract. Several proposed models for dark matter posit the existence of self-interaction processes that can impact the shape of dark matter halos, making them more spherical than the ellipsoidal halos of collisionless dark matter. One method of probing the halo shapes, and thus the strength of the dark matter self-interaction, is by measuring the shape of the X-ray gas that traces the gravitational potential in relaxed elliptical galaxies. In this work we identify a sample of 11 relaxed, isolated elliptical galaxies and measure the ellipticity of the gravitating matter using X-ray images from the XMM-Newton and Chandra telescopes. We explore a variety of different mass configurations and find that the dark matter halos of these galaxies have ellipticities around 0:2 0:5. While we find non-negligible scatter in the ≈ − ellipticity distribution, our results are consistent with some degree of self-interaction at the scale of σ=m 1 cm2/g, yet they also remain compatible with a cold dark matter scenario. ∼ We additionally demonstrate how our results can be used to directly constrain specific dark matter models and discuss implications for current and future simulations of self-interacting dark matter models. -
Modified Newtonian Dynamics
Faculty of Mathematics and Natural Sciences Bachelor Thesis University of Groningen Modified Newtonian Dynamics (MOND) and a Possible Microscopic Description Author: Supervisor: L.M. Mooiweer prof. dr. E. Pallante Abstract Nowadays, the mass discrepancy in the universe is often interpreted within the paradigm of Cold Dark Matter (CDM) while other possibilities are not excluded. The main idea of this thesis is to develop a better theoretical understanding of the hidden mass problem within the paradigm of Modified Newtonian Dynamics (MOND). Several phenomenological aspects of MOND will be discussed and we will consider a possible microscopic description based on quantum statistics on the holographic screen which can reproduce the MOND phenomenology. July 10, 2015 Contents 1 Introduction 3 1.1 The Problem of the Hidden Mass . .3 2 Modified Newtonian Dynamics6 2.1 The Acceleration Constant a0 .................................7 2.2 MOND Phenomenology . .8 2.2.1 The Tully-Fischer and Jackson-Faber relation . .9 2.2.2 The external field effect . 10 2.3 The Non-Relativistic Field Formulation . 11 2.3.1 Conservation of energy . 11 2.3.2 A quadratic Lagrangian formalism (AQUAL) . 12 2.4 The Relativistic Field Formulation . 13 2.5 MOND Difficulties . 13 3 A Possible Microscopic Description of MOND 16 3.1 The Holographic Principle . 16 3.2 Emergent Gravity as an Entropic Force . 16 3.2.1 The connection between the bulk and the surface . 18 3.3 Quantum Statistical Description on the Holographic Screen . 19 3.3.1 Two dimensional quantum gases . 19 3.3.2 The connection with the deep MOND limit . -
Dark Matter, Infinite Statistics, and Quantum Gravity Chiu Man Ho, Djordje Minic, and Y
This is the accepted manuscript made available via CHORUS, the article has been published as: Dark matter, infinite statistics, and quantum gravity Chiu Man Ho, Djordje Minic, and Y. Jack Ng Phys. Rev. D 85, 104033 — Published 21 May 2012 DOI: 10.1103/PhysRevD.85.104033 Dark Matter, Infinite Statistics and Quantum Gravity Chiu Man Ho1∗, Djordje Minic2†, and Y. Jack Ng3‡ 1Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, U.S.A. 2Department of Physics, Virginia Tech, Blacksburg, VA 24061, U.S.A. 3Institute of Field Physics, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599, U.S.A. Abstract We elaborate on our proposal regarding a connection between global physics and local galactic dynamics via quantum gravity. This proposal calls for the concept of MONDian dark matter which behaves like cold dark matter at cluster and cosmological scales but emulates modified Newtonian dynamics (MOND) at the galactic scale. In the present paper, we first point out a surprising connection between the MONDian dark matter and an effective gravitational Born-Infeld theory. We then argue that these unconventional quanta of MONDian dark matter must obey infinite statistics, and the theory must be fundamentally non-local. Finally, we provide a possible top- down approach to our proposal from the Matrix theory point of view. PACS Numbers: 95.35.+d; 04.50.Kd; 05.30.-d; 04.60.-m ∗[email protected] †[email protected] ‡[email protected] 1 1 Introduction The fascinating problem of “missing mass”, or dark matter [1], has been historically iden- tified on the level of galaxies. -
Explosion of the Science Modification of Newtonian Dynamics Via Mach's
Physics International Original Research Paper Explosion of the Science Modification of Newtonian Dynamics Via Mach’s Inertia Principle and Generalization in Gravitational Quantum Bound Systems and Finite Range of the Gravity-Carriers, Consistent Merely On the Bosons and the Fermions Mohsen Lutephy Faculty of Science, Azad Islamic University (IAU), South Tehran branch, Iran Article history Abstract: Newtonian gravity is modified here via Mach's inertia principle Received: 29-04-2020 (inertia fully governed by universe) and it is generalized to gravitationally Revised: 11-05-2020 quantum bound systems, resulting scale invariant fully relational dynamics Accepted: 24-06-2020 (mere ordering upon actual objects), answering to rotation curves and velocity dispersions of the galaxies and clusters (large scale quantum bound Email: [email protected] systems), successful in all dimensions and scales from particle to the universe. Against the Milgrom’s theory, no fundamental acceleration to separate the physical systems to the low and large accelerations, on the contrary the Newtonian regime of HSB galaxies sourced by natural inertia constancy there. All phenomenological paradigms are argued here via Machian modified gravity generalized to quantum gravity, especially Milgrom empirical paradigms and even we have resolved the mystery of missing dark matter in newly discovered Ultra Diffuse Galaxies (UDGs) for potential hollow in host galaxy generated by sub quantum bound system of the globular clusters. Also we see that the strong nuclear force (Yukawa force) is in reality, the enhanced gravity for limitation of the gravitational potential because finite-range of the Compton wavelength of hadronic gravity-carriers in the nucleuses, reasoning to resolve ultimately, one of the biggest questions in the physics, that is, so called the fine structure constant and answering to mysterious saturation features of the nuclear forces and we have resolved also the mystery of the proton stability, reasonable as a quantum micro black hole and the exact calculation of the universe matter. -
Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions Benoit Famaey, Stacy S
Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions Benoit Famaey, Stacy S. Mcgaugh To cite this version: Benoit Famaey, Stacy S. Mcgaugh. Modified Newtonian Dynamics (MOND): Observational Phe- nomenology and Relativistic Extensions. Living Reviews in Relativity, 2012, 15 (1), 10.12942/lrr- 2012-10. hal-02927744 HAL Id: hal-02927744 https://hal.archives-ouvertes.fr/hal-02927744 Submitted on 1 Sep 2020 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. Living Rev. Relativity, 15, (2012), 10 LIVINGREVIEWS http://www.livingreviews.org/lrr-2012-10 in relativity Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions Beno^ıtFamaey Observatoire Astronomique de Strasbourg CNRS, UMR 7550, France and AIfA, University of Bonn, Germany email: [email protected] http://astro.u-strasbg.fr/~famaey/ Stacy S. McGaugh Department of Astronomy University of Maryland, USA and Case Western Reserve University, USA email: [email protected] http://astroweb.case.edu/ssm/ Accepted on 30 April 2012 Published on 7 September 2012 Abstract A wealth of astronomical data indicate the presence of mass discrepancies in the Universe. The motions observed in a variety of classes of extragalactic systems exceed what can be explained by the mass visible in stars and gas. -
What Is Real?
WHAT IS REAL? Space -Time Singularities or Quantum Black Holes? Dark Matter or Planck Mass Particles? General Relativity or Quantum Gravity? Volume or Area Entropy Law? BALUNGI FRANCIS Copyright © BalungiFrancis, 2020 The moral right of the author has been asserted. All rights reserved. Apart from any fair dealing for the purposes of research or private study or critism or review, no part of this publication may be reproduced, distributed, or transmitted in any form or by any means, including photocopying, recording, or other electronic or mechanical methods, or by any information storage and retrieval system without the prior written permission of the publisher. TABLE OF CONTENTS TABLE OF CONTENTS i DEDICATION 1 PREFACE ii Space-time Singularity or Quantum Black Holes? Error! Bookmark not defined. What is real? Is it Volume or Area Entropy Law of Black Holes? 1 Is it Dark Matter, MOND or Quantum Black Holes? 6 What is real? General Relativity or Quantum Gravity Error! Bookmark not defined. Particle Creation by Black Holes: Is it Hawking’s Approach or My Approach? Error! Bookmark not defined. Stellar Mass Black Holes or Primordial Holes Error! Bookmark not defined. Additional Readings Error! Bookmark not defined. Hidden in Plain sight1: A Simple Link between Quantum Mechanics and Relativity Error! Bookmark not defined. Hidden in Plain sight2: From White Dwarfs to Black Holes Error! Bookmark not defined. Appendix 1 Error! Bookmark not defined. Derivation of the Energy density stored in the Electric field and Gravitational Field Error! -
Astro-Ph.CO] 13 Sep 2017 1
September 14, 2017 0:22 WSPC/INSTRUCTION FILE MDMreview_20170908 International Journal of Modern Physics D c World Scientific Publishing Company Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter Douglas Edmonds1∗, 2, Duncan Farrah2y, Djordje Minic2z, Y. Jack Ng3x, and Tatsu Takeuchi2{ 1Department of Physics, The Pennsylvania State University, Hazleton, PA 18202 USA, 2Department of Physics, Center for Neutrino Physics, Virginia Tech, Blacksburg, VA 24061 USA, 3Institute of Field Physics, Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599 USA ∗[email protected], [email protected], [email protected], [email protected], {[email protected] Received Day Month Year Revised Day Month Year Modified dark matter (MDM) is a phenomenological model of dark matter, inspired by gravitational thermodynamics. For an accelerating Universe with positive cosmo- logical constant (Λ), such phenomenological considerations lead to the emergence of a critical acceleration parameter related to Λ. Such a critical acceleration is an effective phenomenological manifestation of MDM, and it is found in correlations between dark matter and baryonic matter in galaxy rotation curves. The resulting MDM mass profiles, which are sensitive to Λ, are consistent with observational data at both the galactic and cluster scales. In particular, the same critical acceleration appears both in the galactic and cluster data fits based on MDM. Furthermore, using some robust qualitative ar- guments, MDM appears to work well on cosmological scales, even though quantitative studies are still lacking. Finally, we comment on certain non-local aspects of the quanta of modified dark matter, which may lead to novel non-particle phenomenology and which may explain why, so far, dark matter detection experiments have failed to detect dark matter particles. -
Arxiv:Astro-Ph/0701848V1 30 Jan 2007 Xetd Tesaclrto Eas Ti H Quantity the Is It Because Than Acceleration Bigger Stress Much I Are Velocities Expected
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server The modified Newtonian dynamics—MOND and its implications for new physics Jacob D. Bekenstein∗ No more salient issue exists in contemporary astrophysics and cosmology than that of the elusive “dark matter”. For many years already Milgrom’s paradigm of modified Newtonian dynamics (MOND) has provided an alternative way to interpret observations without appeal to invisible dark matter. MOND had been successful in elucidating economically the dynamics of disk galaxies of all scales, while doing less well for clusters of galaxies; in its original form it could not address gravitational lensing or cosmology. After reviewing some of the evidence in favor of MOND, I recollect the development of relativistic formulations for it to cope with the last deficiency. I comment on recent work by various groups in confronting TeVeS, a relativistic embodiment of MOND, with observational data on gravitational lensing and cosmology. Throughout I ask what sort of physics can be responsible for the efficacy of MOND, and conclude with an appraisal of what theoretical developments are still needed to reach a full description of the world involving no unobserved matter. 1. Introduction which directly measures the strength of the gravitational field. In any case, what is wrong? It was realized by Ostriker and Peebles [1] that mas- Newtonian gravity theory has served physics and tech- sive halos would stabilize disk galaxies against the bar nology faithfully for well over three centuries. Neverthe- forming instabilities which, in Newtonian theory, are en- less, it has long been known that it is only an approxi- demic to systems with little velocity dispersion. -
The Board of Governors
Table of Contents The Board of Governors..........................................................................................................1 The Scientific and Academic Advisory Committee...............................................................9 Institute Officers.....................................................................................................................11 The Weizmann Institute of Science.......................................................................................15 Faculty of Biochemistry.........................................................................................................17 Faculty of Biochemistry...............................................................................................18 Biological Chemistry....................................................................................................20 Molecular Genetics.......................................................................................................30 Plant Sciences...............................................................................................................39 Biological Services.......................................................................................................47 The Avron−Wilstätter Minerva Center for Research in Photosynthesis......................50 The Y. Leon Benoziyo Institute for Molecular Medicine............................................52 The Dr. Josef Cohn Minerva Center for Biomembrane Research................................54 The -
Lagrangian Formulation of Mond; Mond Field in Perturbed Spherical Systems
LAGRANGIAN FORMULATION OF MOND; MOND FIELD IN PERTURBED SPHERICAL SYSTEMS by REIJIRO MATSUO Submitted in partial fulfillment of the requirements For the degree of Doctor of Philosophy Dissertation Adviser: Dr. Glenn Starkman Department of Physics CASE WESTERN RESERVE UNIVERSITY August 2010 CASE WESTERN RESERVE UNIVERSITY SCHOOL OF GRADUATE STUDIES We hereby approve the thesis/dissertation of Reijiro Matsuo candidate for the Doctor of Philosophy degree*. Dr. Glenn Starkman (chair of the committee) Dr. Barry Wessels Dr. Corbin Covault Dr. Harsh Mathur June 29, 2010 Contents 1 Introduction 1 2 Basic theory of MOND and its phenomenological implications 5 2.1 TheOriginalFormulationofMOND . 5 2.2 MONDandrotationcurvefitting . 7 2.3 TheLagrangianFormulationofMOND . 8 2.4 RelativisticFormulationsofMOND . 10 2.5 Confrontations with MOND, X-ray emitting Clusters . ... 14 2.6 Confrontations with MOND, the Bullet Cluster . .. 16 2.6.1 ConditionsonaVectorPerturbation . 18 2.6.2 NumericalCode.......................... 21 2.6.3 LensingandConvergencemap. 22 2.6.4 Model ............................... 26 2.6.5 Result ............................... 31 3 MONDfieldandperturbedsphericalsystems 32 3.1 GeneralSetups .............................. 32 3.2 PerturbationsinsideaMassShell . 35 3.2.1 GeneralRelativity . 35 3.2.2 MOND............................... 37 3.2.3 APerturbativecalculation . 37 3.2.4 Numericalcalculations . 40 3.2.5 TestingtheCode ......................... 41 3.3 PerturbationsonaShellandoutsideaShell . ... 43 3.3.1 ShieldingandAnti-Shieldingeffects