Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Measurement of the Speed of Gravity
Measurement of the Speed of Gravity Yin Zhu Agriculture Department of Hubei Province, Wuhan, China Abstract From the Liénard-Wiechert potential in both the gravitational field and the electromagnetic field, it is shown that the speed of propagation of the gravitational field (waves) can be tested by comparing the measured speed of gravitational force with the measured speed of Coulomb force. PACS: 04.20.Cv; 04.30.Nk; 04.80.Cc Fomalont and Kopeikin [1] in 2002 claimed that to 20% accuracy they confirmed that the speed of gravity is equal to the speed of light in vacuum. Their work was immediately contradicted by Will [2] and other several physicists. [3-7] Fomalont and Kopeikin [1] accepted that their measurement is not sufficiently accurate to detect terms of order , which can experimentally distinguish Kopeikin interpretation from Will interpretation. Fomalont et al [8] reported their measurements in 2009 and claimed that these measurements are more accurate than the 2002 VLBA experiment [1], but did not point out whether the terms of order have been detected. Within the post-Newtonian framework, several metric theories have studied the radiation and propagation of gravitational waves. [9] For example, in the Rosen bi-metric theory, [10] the difference between the speed of gravity and the speed of light could be tested by comparing the arrival times of a gravitational wave and an electromagnetic wave from the same event: a supernova. Hulse and Taylor [11] showed the indirect evidence for gravitational radiation. However, the gravitational waves themselves have not yet been detected directly. [12] In electrodynamics the speed of electromagnetic waves appears in Maxwell equations as c = √휇0휀0, no such constant appears in any theory of gravity. -
Dark Energy and Dark Matter As Inertial Effects Introduction
Dark Energy and Dark Matter as Inertial Effects Serkan Zorba Department of Physics and Astronomy, Whittier College 13406 Philadelphia Street, Whittier, CA 90608 [email protected] ABSTRACT A disk-shaped universe (encompassing the observable universe) rotating globally with an angular speed equal to the Hubble constant is postulated. It is shown that dark energy and dark matter are cosmic inertial effects resulting from such a cosmic rotation, corresponding to centrifugal (dark energy), and a combination of centrifugal and the Coriolis forces (dark matter), respectively. The physics and the cosmological and galactic parameters obtained from the model closely match those attributed to dark energy and dark matter in the standard Λ-CDM model. 20 Oct 2012 Oct 20 ph] - PACS: 95.36.+x, 95.35.+d, 98.80.-k, 04.20.Cv [physics.gen Introduction The two most outstanding unsolved problems of modern cosmology today are the problems of dark energy and dark matter. Together these two problems imply that about a whopping 96% of the energy content of the universe is simply unaccounted for within the reigning paradigm of modern cosmology. arXiv:1210.3021 The dark energy problem has been around only for about two decades, while the dark matter problem has gone unsolved for about 90 years. Various ideas have been put forward, including some fantastic ones such as the presence of ghostly fields and particles. Some ideas even suggest the breakdown of the standard Newton-Einstein gravity for the relevant scales. Although some progress has been made, particularly in the area of dark matter with the nonstandard gravity theories, the problems still stand unresolved. -
Inflation and the Theory of Cosmological Perturbations
Inflation and the Theory of Cosmological Perturbations A. Riotto INFN, Sezione di Padova, via Marzolo 8, I-35131, Padova, Italy. Abstract These lectures provide a pedagogical introduction to inflation and the theory of cosmological per- turbations generated during inflation which are thought to be the origin of structure in the universe. Lectures given at the: Summer School on arXiv:hep-ph/0210162v2 30 Jan 2017 Astroparticle Physics and Cosmology Trieste, 17 June - 5 July 2002 1 Notation A few words on the metric notation. We will be using the convention (−; +; +; +), even though we might switch time to time to the other option (+; −; −; −). This might happen for our convenience, but also for pedagogical reasons. Students should not be shielded too much against the phenomenon of changes of convention and notation in books and articles. Units We will adopt natural, or high energy physics, units. There is only one fundamental dimension, energy, after setting ~ = c = kb = 1, [Energy] = [Mass] = [Temperature] = [Length]−1 = [Time]−1 : The most common conversion factors and quantities we will make use of are 1 GeV−1 = 1:97 × 10−14 cm=6:59 × 10−25 sec, 1 Mpc= 3.08×1024 cm=1.56×1038 GeV−1, 19 MPl = 1:22 × 10 GeV, −1 −1 −42 H0= 100 h Km sec Mpc =2.1 h × 10 GeV, 2 −29 −3 2 4 −3 2 −47 4 ρc = 1:87h · 10 g cm = 1:05h · 10 eV cm = 8:1h × 10 GeV , −13 T0 = 2:75 K=2.3×10 GeV, 2 Teq = 5:5(Ω0h ) eV, Tls = 0:26 (T0=2:75 K) eV. -
Hypercomplex Algebras and Their Application to the Mathematical
Hypercomplex Algebras and their application to the mathematical formulation of Quantum Theory Torsten Hertig I1, Philip H¨ohmann II2, Ralf Otte I3 I tecData AG Bahnhofsstrasse 114, CH-9240 Uzwil, Schweiz 1 [email protected] 3 [email protected] II info-key GmbH & Co. KG Heinz-Fangman-Straße 2, DE-42287 Wuppertal, Deutschland 2 [email protected] March 31, 2014 Abstract Quantum theory (QT) which is one of the basic theories of physics, namely in terms of ERWIN SCHRODINGER¨ ’s 1926 wave functions in general requires the field C of the complex numbers to be formulated. However, even the complex-valued description soon turned out to be insufficient. Incorporating EINSTEIN’s theory of Special Relativity (SR) (SCHRODINGER¨ , OSKAR KLEIN, WALTER GORDON, 1926, PAUL DIRAC 1928) leads to an equation which requires some coefficients which can neither be real nor complex but rather must be hypercomplex. It is conventional to write down the DIRAC equation using pairwise anti-commuting matrices. However, a unitary ring of square matrices is a hypercomplex algebra by definition, namely an associative one. However, it is the algebraic properties of the elements and their relations to one another, rather than their precise form as matrices which is important. This encourages us to replace the matrix formulation by a more symbolic one of the single elements as linear combinations of some basis elements. In the case of the DIRAC equation, these elements are called biquaternions, also known as quaternions over the complex numbers. As an algebra over R, the biquaternions are eight-dimensional; as subalgebras, this algebra contains the division ring H of the quaternions at one hand and the algebra C ⊗ C of the bicomplex numbers at the other, the latter being commutative in contrast to H. -
Fine-Tuning, Complexity, and Life in the Multiverse*
Fine-Tuning, Complexity, and Life in the Multiverse* Mario Livio Dept. of Physics and Astronomy, University of Nevada, Las Vegas, NV 89154, USA E-mail: [email protected] and Martin J. Rees Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, UK E-mail: [email protected] Abstract The physical processes that determine the properties of our everyday world, and of the wider cosmos, are determined by some key numbers: the ‘constants’ of micro-physics and the parameters that describe the expanding universe in which we have emerged. We identify various steps in the emergence of stars, planets and life that are dependent on these fundamental numbers, and explore how these steps might have been changed — or completely prevented — if the numbers were different. We then outline some cosmological models where physical reality is vastly more extensive than the ‘universe’ that astronomers observe (perhaps even involving many ‘big bangs’) — which could perhaps encompass domains governed by different physics. Although the concept of a multiverse is still speculative, we argue that attempts to determine whether it exists constitute a genuinely scientific endeavor. If we indeed inhabit a multiverse, then we may have to accept that there can be no explanation other than anthropic reasoning for some features our world. _______________________ *Chapter for the book Consolidation of Fine Tuning 1 Introduction At their fundamental level, phenomena in our universe can be described by certain laws—the so-called “laws of nature” — and by the values of some three dozen parameters (e.g., [1]). Those parameters specify such physical quantities as the coupling constants of the weak and strong interactions in the Standard Model of particle physics, and the dark energy density, the baryon mass per photon, and the spatial curvature in cosmology. -
Galaxy Redshifts: from Dozens to Millions
GALAXY REDSHIFTS: FROM DOZENS TO MILLIONS Chris Impey University of Arizona The Expanding Universe • Evolution of the scale factor from GR; metric assumes homogeneity and isotropy (~FLRW). • Cosmological redshift fundamentally differs from a Doppler shift. • Galaxies (and other objects) are used as space-time markers. Expansion History and Contents Science is Seeing The expansion history since the big bang and the formation of large scale structure are driven by dark matter and dark energy. Observing Galaxies Galaxy Observables: • Redshift (z) • Magnitude (color, SED) • Angular size (morphology) All other quantities (size, luminosity, mass) derive from knowing a distance, which relates to redshift via a cosmological model. The observables are poor distance indicators. Other astrophysical luminosity predictors are required. (Cowie) ~90% of the volume or look-back time is probed by deep field • Number of galaxies in observable universe: ~90% of the about 100 billion galaxies in the volume • Number of stars in the are counted observable universe: about 1022 Heading for 100 Million (Baldry/Eisenstein) Multiplex Advantage Cannon (1910) Gemini/GMOS (2010) Sluggish, Spacious, Reliable. Photography CCD Imaging Speedy, Cramped, Finicky. 100 Years of Measuring Galaxy Redshifts Who When # Galaxies Size Time Mag Scheiner 1899 1 (M31) 0.3m 7.5h V = 3.4 Slipher 1914 15 0.6m ~5h V ~ 8 Slipher 1917 25 0.6m ~5h V ~ 8 Hubble/Slipher 1929 46 1.5m ~6h V ~ 10 Hum/May/San 1956 800 5m ~2h V = 11.6 Photographic 1960s 1 ~4m ~2.5h V ~ 15 Image Intensifier 1970s -
New Constraints on Cosmic Reionization
New Constraints on Cosmic Reionization Brant Robertson UCSC Exploring the Universe with JWST ESA / ESTEC, The Netherlands October 12, 2015 1 Exploring the Universe with JWST, 10/12/2015 B. Robertson, UCSC Brief History of the Observable Universe 1100 Redshift 12 8 6 1 13.8 13.5 Billions of years ago 13.4 12.9 8 Adapted from Robertson et al. Nature, 468, 49 (2010). 2 Exploring the Universe with JWST, 10/12/2015 B. Robertson, UCSC Observational Facilities Over the Next Decade 1100 Redshift 12 8 6 1 Planck Future 21cm Current 21cm LSST Thirty Meter Telescope WFIRST ALMA Hubble Chandra Fermi James Webb Space Telescope 13.8 13.5 Billions of years ago 13.4 12.9 8 Observations with JWST, WFIRST, TMT/E-ELT, LSST, ALMA, and 21- cm will drive astronomical discoveries over the next decade. Adapted from Robertson et al. Nature, 468, 49 (2010). 3 Exploring the Universe with JWST, 10/12/2015 B. Robertson, UCSC 1100 Redshift 12 8 6 1 Planck Future 21cm Current 21cm LSST Thirty Meter Telescope WFIRST ALMA Hubble Chandra Fermi James Webb Space Telescope 13.8 13.5 Billions of years ago 13.4 12.9 8 1. What can we learn about Cosmic Dawn? Was it a dramatic event in a narrow period of time or did the birth of galaxies happen gradually? 2. Can we be sure light from early galaxies caused cosmic reionization? We have some guide on when reionization occurred from studying the thermal glow of the Big Bang (microwave background), but what were the sources of ionizing photons? 3. -
Experimental Determination of the Speed of Light by the Foucault Method
Experimental Determination of the Speed of Light by the Foucault Method R. Price and J. Zizka University of Arizona The speed of light was measured using the Foucault method of reflecting a beam of light from a rotating mirror to a fixed mirror and back creating two separate reflected beams with an angular displacement that is related to the time that was required for the light beam to travel a given distance to the fixed mirror. By taking measurements relating the displacement of the two light beams and the angular speed of the rotating mirror, the speed of light was found to be (3.09±0.204)x108 m/s, which is within 2.7% of the defined value for the speed of light. 1 Introduction The goal of the experiment was to experimentally measure the speed of light, c, in a vacuum by using the Foucault method for measuring the speed of light. Although there are many experimental methods available to measure the speed of light, the underlying principle behind all methods on the simple kinematic relationship between constant velocity, distance and time given below: D c = (1) t In all forms of the experiment, the objective is to measure the time required for the light to travel a given distance. The large magnitude of the speed of light prevents any direct measurements of the time a light beam going across a given distance similar to kinematic experiments. Galileo himself attempted such an experiment by having two people hold lights across a distance. One of the experiments would put out their light and when the second observer saw the light cease, they would put out theirs. -
The Reionization of Cosmic Hydrogen by the First Galaxies Abstract 1
David Goodstein’s Cosmology Book The Reionization of Cosmic Hydrogen by the First Galaxies Abraham Loeb Department of Astronomy, Harvard University, 60 Garden St., Cambridge MA, 02138 Abstract Cosmology is by now a mature experimental science. We are privileged to live at a time when the story of genesis (how the Universe started and developed) can be critically explored by direct observations. Looking deep into the Universe through powerful telescopes, we can see images of the Universe when it was younger because of the finite time it takes light to travel to us from distant sources. Existing data sets include an image of the Universe when it was 0.4 million years old (in the form of the cosmic microwave background), as well as images of individual galaxies when the Universe was older than a billion years. But there is a serious challenge: in between these two epochs was a period when the Universe was dark, stars had not yet formed, and the cosmic microwave background no longer traced the distribution of matter. And this is precisely the most interesting period, when the primordial soup evolved into the rich zoo of objects we now see. The observers are moving ahead along several fronts. The first involves the construction of large infrared telescopes on the ground and in space, that will provide us with new photos of the first galaxies. Current plans include ground-based telescopes which are 24-42 meter in diameter, and NASA’s successor to the Hubble Space Telescope, called the James Webb Space Telescope. In addition, several observational groups around the globe are constructing radio arrays that will be capable of mapping the three-dimensional distribution of cosmic hydrogen in the infant Universe. -
Evolution of the Cosmological Horizons in a Concordance Universe
Evolution of the Cosmological Horizons in a Concordance Universe Berta Margalef–Bentabol 1 Juan Margalef–Bentabol 2;3 Jordi Cepa 1;4 [email protected] [email protected] [email protected] 1Departamento de Astrofísica, Universidad de la Laguna, E-38205 La Laguna, Tenerife, Spain: 2Facultad de Ciencias Matemáticas, Universidad Complutense de Madrid, E-28040 Madrid, Spain. 3Facultad de Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain. 4Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain. Abstract The particle and event horizons are widely known and studied concepts, but the study of their properties, in particular their evolution, have only been done so far considering a single state equation in a deceler- ating universe. This paper is the first of two where we study this problem from a general point of view. Specifically, this paper is devoted to the study of the evolution of these cosmological horizons in an accel- erated universe with two state equations, cosmological constant and dust. We have obtained closed-form expressions for the horizons, which have allowed us to compute their velocities in terms of their respective recession velocities that generalize the previous results for one state equation only. With the equations of state considered, it is proved that both velocities remain always positive. Keywords: Physics of the early universe – Dark energy theory – Cosmological simulations This is an author-created, un-copyedited version of an article accepted for publication in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd/SISSA Medialab srl is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. -
The Age of the Universe, the Hubble Constant, the Accelerated Expansion and the Hubble Effect
The age of the universe, the Hubble constant, the accelerated expansion and the Hubble effect Domingos Soares∗ Departamento de F´ısica,ICEx, UFMG | C.P. 702 30123-970, Belo Horizonte | Brazil October 25, 2018 Abstract The idea of an accelerating universe comes almost simultaneously with the determination of Hubble's constant by one of the Hubble Space Tele- scope Key Projects. The age of the universe dilemma is probably the link between these two issues. In an appendix, I claim that \Hubble's law" might yet to be investigated for its ultimate cause, and suggest the \Hubble effect” as the searched candidate. 1 The age dilemma The age of the universe is calculated by two different ways. Firstly, a lower limit is given by the age of the presumably oldest objects in the Milky Way, e.g., globular clusters. Their ages are calculated with the aid of stellar evolu- tion models which yield 14 Gyr and 10% uncertainty. These are fairly confident figures since the basics of stellar evolution are quite solid. Secondly, a cosmo- logical age based on the Standard Cosmology Model derived from the Theory of General Relativity. The three basic models of relativistic cosmology are given by the Friedmann's solutions of Einstein's field equations. The models are char- acterized by a decelerated expansion from a spatial singularity at cosmic time t = 0, and whose magnitude is quantified by the density parameter Ω◦, the present ratio of the mass density in the universe to the so-called critical mass arXiv:0908.1864v8 [physics.gen-ph] 28 Jul 2015 density. -
Albert Einstein's Key Breakthrough — Relativity
{ EINSTEIN’S CENTURY } Albert Einstein’s key breakthrough — relativity — came when he looked at a few ordinary things from a different perspective. /// BY RICHARD PANEK Relativity turns 1001 How’d he do it? This question has shadowed Albert Einstein for a century. Sometimes it’s rhetorical — an expression of amazement that one mind could so thoroughly and fundamentally reimagine the universe. And sometimes the question is literal — an inquiry into how Einstein arrived at his special and general theories of relativity. Einstein often echoed the first, awestruck form of the question when he referred to the mind’s workings in general. “What, precisely, is ‘thinking’?” he asked in his “Autobiographical Notes,” an essay from 1946. In somebody else’s autobiographical notes, even another scientist’s, this question might have been unusual. For Einstein, though, this type of question was typical. In numerous lectures and essays after he became famous as the father of relativity, Einstein began often with a meditation on how anyone could arrive at any subject, let alone an insight into the workings of the universe. An answer to the literal question has often been equally obscure. Since Einstein emerged as a public figure, a mythology has enshrouded him: the lone- ly genius sitting in the patent office in Bern, Switzerland, thinking his little thought experiments until one day, suddenly, he has a “Eureka!” moment. “Eureka!” moments young Einstein had, but they didn’t come from nowhere. He understood what scientific questions he was trying to answer, where they fit within philosophical traditions, and who else was asking them.