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October 2020 Deirdre Shoemaker, Ph.D. Center for Gravitational Physics Department of Physics University of Texas at Austin Google Scholar
October 2020 Deirdre Shoemaker, Ph.D. Center for Gravitational Physics Department of Physics University of Texas at Austin Google scholar: http://bit.ly/1FIoCFf I. Earned Degrees B.S. Astronomy & Astrophysics 1990-1994 Pennsylvania State University with Honors and Physics Ph.D. Physics 1995-1999 University of Texas at Austin (advisor: R. Matzner) II. Employment History 1999-2002 Postdoctoral Fellow, Center for Gravitational Wave Physics, Penn State (advisor: S. Finn and J. Pullin) 2002-2004 Research Associate, Center for Radiophysics and Space Research, Cornell (advisor: S. Teukolsky) 2004-2008 Assistant Professor, Physics, Penn State 2008-2011 Assistant Professor, Physics, Georgia Institute of Technology 2009-2011 Adjunct Assistant Professor, School of Computational Science and Engineering, Georgia Institute of Technology 2011-2016 Associate Professor, Physics, Georgia Institute of Technology 2011-2016 Adjunct Associate Professor, School of Computational Science and Engineering, Georgia Institute of Technology 2013-2020 Director, Center for Relativistic Astrophysics 2016-2020 Professor, Physics, Georgia Institute of Technology 2016-2020 Adjunct Professor, School of Computational Science and Engineering, Georgia Institute of Technology 2017-2020 Associate Director of Research and Strategic Initiatives, Institute of Data, Engineering and Science, Georgia Institute of Technology 2020-Present Professor, Physics, University of Texas at Austin 2020-Present Director, Center for Gravitational Physics, University of Texas at Austin III. Honors -
Arxiv:2012.00011V2 [Astro-Ph.HE] 20 Dec 2020 Mergers in Gas-Rich Environments (Mckernan Et Al
Draft version December 22, 2020 Preprint typeset using LATEX style emulateapj v. 12/16/11 MASS-GAP MERGERS IN ACTIVE GALACTIC NUCLEI Hiromichi Tagawa1, Bence Kocsis2, Zoltan´ Haiman3, Imre Bartos4, Kazuyuki Omukai1, Johan Samsing5 1Astronomical Institute, Graduate School of Science, Tohoku University, Aoba, Sendai 980-8578, Japan 2 Rudolf Peierls Centre for Theoretical Physics, Clarendon Laboratory, Parks Road, Oxford OX1 3PU, UK 3Department of Astronomy, Columbia University, 550 W. 120th St., New York, NY, 10027, USA 4Department of Physics, University of Florida, PO Box 118440, Gainesville, FL 32611, USA 5Niels Bohr International Academy, The Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark Draft version December 22, 2020 ABSTRACT The recently discovered gravitational wave sources GW190521 and GW190814 have shown evidence of BH mergers with masses and spins outside of the range expected from isolated stellar evolution. These merging objects could have undergone previous mergers. Such hierarchical mergers are predicted to be frequent in active galactic nuclei (AGN) disks, where binaries form and evolve efficiently by dynamical interactions and gaseous dissipation. Here we compare the properties of these observed events to the theoretical models of mergers in AGN disks, which are obtained by performing one-dimensional N- body simulations combined with semi-analytical prescriptions. The high BH masses in GW190521 are consistent with mergers of high-generation (high-g) BHs where the initial progenitor stars had high metallicity, 2g BHs if the original progenitors were metal-poor, or 1g BHs that had gained mass via super-Eddington accretion. Other measured properties related to spin parameters in GW190521 are also consistent with mergers in AGN disks. -
Midwife of the Galactic Zoo
FOCUS 30 A miniature milky way: approximately 40 million light-years away, UGC 5340 is classified as a dwarf galaxy. Dwarf galaxies exist in a variety of forms – elliptical, spheroidal, spiral, or irregular – and originate in small halos of dark matter. Dwarf galaxies contain the oldest known stars. Max Planck Research · 4 | 2020 FOCUS MIDWIFE OF THE GALACTIC ZOO TEXT: THOMAS BÜHRKE 31 IMAGE: NASA, TEAM ESA & LEGUS Stars cluster in galaxies of dramatically different shapes and sizes: elliptical galaxies, spheroidal galaxies, lenticular galaxies, spiral galaxies, and occasionally even irregular galaxies. Nadine Neumayer at the Max Planck Institute for Astronomy in Heidelberg and Ralf Bender at the Max Planck Institute for Extraterrestrial Physics in Garching investigate the reasons for this diversity. They have already identified one crucial factor: dark matter. Max Planck Research · 4 | 2020 FOCUS Nature has bestowed an overwhelming diversity upon our planet. The sheer resourcefulness of the plant and animal world is seemingly inexhaustible. When scien- tists first started to explore this diversity, their first step was always to systematize it. Hence, the Swedish naturalist Carl von Linné established the principles of modern botany and zoology in the 18th century by clas- sifying organisms. In the last century, astronomers have likewise discovered that galaxies can come in an array of shapes and sizes. In this case, it was Edwin Hubble in the mid-1920s who systematized them. The “Hubble tuning fork dia- gram” classified elliptical galaxies according to their ellipticity. The series of elliptical galaxies along the di- PHOTO: PETER FRIEDRICH agram branches off into two arms: spiral galaxies with a compact bulge along the upper branch and galaxies with a central bar on the lower branch. -
Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects
Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Porto Alegre 2017 Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Dissertação elaborada sob orientação do Prof. Dr. Eduardo Luis Damiani Bica, co- orientação do Prof. Dr. Charles José Bon- ato e apresentada ao Instituto de Física da Universidade Federal do Rio Grande do Sul em preenchimento do requisito par- cial para obtenção do título de Mestre em Física. Porto Alegre 2017 Acknowledgements To my parents, who supported me and made this possible, in a time and place where being in a university was just a distant dream. To my dearest friends Elisabeth, Robert, Augusto, and Natália - who so many times helped me go from "I give up" to "I’ll try once more". To my cats Kira, Fen, and Demi - who lazily join me in bed at the end of the day, and make everything worthwhile. "But, first of all, it will be necessary to explain what is our idea of a cluster of stars, and by what means we have obtained it. For an instance, I shall take the phenomenon which presents itself in many clusters: It is that of a number of lucid spots, of equal lustre, scattered over a circular space, in such a manner as to appear gradually more compressed towards the middle; and which compression, in the clusters to which I allude, is generally carried so far, as, by imperceptible degrees, to end in a luminous center, of a resolvable blaze of light." William Herschel, 1789 Abstract We provide a sample of 170 Galactic Globular Clusters (GCs) and analyse its spatial distribution properties. -
Einstein's Geometrical Versus Feynman's Quantum-Field
Universe 2020, 6(11), 212; doi:10.3390/universe6110212 Einstein’s Geometrical Versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy Yurij Baryshev 1, ∗ 1Astronomy Department, Mathematics & Mechanics Faculty, Saint Petersburg State University, 28 Universitetskiy Prospekt, 198504 St. Petersburg, Russia Modern multimessenger astronomy delivers unique opportunity for performing crucial ob- servations that allow for testing the physics of the gravitational interaction. These tests include detection of gravitational waves by advanced LIGO-Virgo antennas, Event Horizon Telescope observations of central relativistic compact objects (RCO) in active galactic nuclei (AGN), X-ray spectroscopic observations of Fe Kα line in AGN, Galactic X-ray sources mea- surement of masses and radiuses of neutron stars, quark stars, and other RCO. A very impor- tant task of observational cosmology is to perform large surveys of galactic distances indepen- dent on cosmological redshifts for testing the nature of the Hubble law and peculiar velocities. Forthcoming multimessenger astronomy, while using such facilities as advanced LIGO-Virgo, Event Horizon Telescope (EHT), ALMA, WALLABY, JWST, EUCLID, and THESEUS, can elucidate the relation between Einstein’s geometrical and Feynman’s quantum-field ap- proaches to gravity physics and deliver a new possibilities for unification of gravitation with other fundamental quantum physical interactions. Keywords: gravitation; cosmology; multimessenger astronomy; quantum physics. arXiv:1702.02020v3 [physics.gen-ph] 4 Dec 2020 ∗ Electronic address: [email protected]; [email protected] 2 Contents 1. Introduction 5 1.1. Key Discoveries of Modern Multimessenger Astronomy 6 1. Gravitational Waves 6 2. Imaging of Black Holes Candidates: Relativistic Jets and Disks 7 3. -
GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole 4 with a 2.6 M Compact Object
1 Draft version May 21, 2020 2 Typeset using LATEX twocolumn style in AASTeX63 3 GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole 4 with a 2.6 M Compact Object 5 LIGO Scientific Collaboration and Virgo Collaboration 6 7 (Dated: May 21, 2020) 8 ABSTRACT 9 We report the observation of a compact binary coalescence involving a 22.2 { 24.3 M black hole and 10 a compact object with a mass of 2.50 { 2.67 M (all measurements quoted at the 90% credible level). 11 The gravitational-wave signal, GW190814, was observed during LIGO's and Virgo's third observing 12 run on August 14, 2019 at 21:10:39 UTC and has a signal-to-noise ratio of 25 in the three-detector 2 +41 13 network. The source was localized to 18.5 deg at a distance of 241−45 Mpc; no electromagnetic 14 counterpart has been confirmed to date. The source has the most unequal mass ratio yet measured +0:008 15 with gravitational waves, 0:112−0:009, and its secondary component is either the lightest black hole 16 or the heaviest neutron star ever discovered in a double compact-object system. The dimensionless 17 spin of the primary black hole is tightly constrained to 0:07. Tests of general relativity reveal no ≤ 18 measurable deviations from the theory, and its prediction of higher-multipole emission is confirmed at −3 −1 19 high confidence. We estimate a merger rate density of 1{23 Gpc yr for the new class of binary 20 coalescence sources that GW190814 represents. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Probing the Nuclear Equation of State from the Existence of a 2.6 M Neutron Star: the GW190814 Puzzle
S S symmetry Article Probing the Nuclear Equation of State from the Existence of a ∼2.6 M Neutron Star: The GW190814 Puzzle Alkiviadis Kanakis-Pegios †,‡ , Polychronis S. Koliogiannis ∗,†,‡ and Charalampos C. Moustakidis †,‡ Department of Theoretical Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece; [email protected] (A.K.P.); [email protected] (C.C.M.) * Correspondence: [email protected] † Current address: Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece. ‡ These authors contributed equally to this work. Abstract: On 14 August 2019, the LIGO/Virgo collaboration observed a compact object with mass +0.08 2.59 0.09 M , as a component of a system where the main companion was a black hole with mass ∼ − 23 M . A scientific debate initiated concerning the identification of the low mass component, as ∼ it falls into the neutron star–black hole mass gap. The understanding of the nature of GW190814 event will offer rich information concerning open issues, the speed of sound and the possible phase transition into other degrees of freedom. In the present work, we made an effort to probe the nuclear equation of state along with the GW190814 event. Firstly, we examine possible constraints on the nuclear equation of state inferred from the consideration that the low mass companion is a slow or rapidly rotating neutron star. In this case, the role of the upper bounds on the speed of sound is revealed, in connection with the dense nuclear matter properties. Secondly, we systematically study the tidal deformability of a possible high mass candidate existing as an individual star or as a component one in a binary neutron star system. -
Recent Observations of Gravitational Waves by LIGO and Virgo Detectors
universe Review Recent Observations of Gravitational Waves by LIGO and Virgo Detectors Andrzej Królak 1,2,* and Paritosh Verma 2 1 Institute of Mathematics, Polish Academy of Sciences, 00-656 Warsaw, Poland 2 National Centre for Nuclear Research, 05-400 Otwock, Poland; [email protected] * Correspondence: [email protected] Abstract: In this paper we present the most recent observations of gravitational waves (GWs) by LIGO and Virgo detectors. We also discuss contributions of the recent Nobel prize winner, Sir Roger Penrose to understanding gravitational radiation and black holes (BHs). We make a short introduction to GW phenomenon in general relativity (GR) and we present main sources of detectable GW signals. We describe the laser interferometric detectors that made the first observations of GWs. We briefly discuss the first direct detection of GW signal that originated from a merger of two BHs and the first detection of GW signal form merger of two neutron stars (NSs). Finally we present in more detail the observations of GW signals made during the first half of the most recent observing run of the LIGO and Virgo projects. Finally we present prospects for future GW observations. Keywords: gravitational waves; black holes; neutron stars; laser interferometers 1. Introduction The first terrestrial direct detection of GWs on 14 September 2015, was a milestone Citation: Kro´lak, A.; Verma, P. discovery, and it opened up an entirely new window to explore the universe. The combined Recent Observations of Gravitational effort of various scientists and engineers worldwide working on the theoretical, experi- Waves by LIGO and Virgo Detectors. -
Many New Variable Stars Discovered in the Core of the Globular Cluster NGC 6715 (M 54) with EMCCD Observations DOI: 10.1051/0004-6361/201628864
The University of Manchester Research Many new variable stars discovered in the core of the globular cluster NGC 6715 (M 54) with EMCCD observations DOI: 10.1051/0004-6361/201628864 Document Version Accepted author manuscript Link to publication record in Manchester Research Explorer Citation for published version (APA): Figuera Jaimes, R., Bramich, D. M., Kains, N., Skottfelt, J., Jørgensen, U. G., Horne, K., Dominik, M., Alsubai, K. A., Bozza, V., Burgdorf, M. J., Calchi Novati, S., Ciceri, S., D'Ago, G., Evans, D. F., Galianni, P., Gu, S. H., W Harpsøe, K. B., Haugbølle, T., Hinse, T. C., ... Wertz, O. (2016). Many new variable stars discovered in the core of the globular cluster NGC 6715 (M 54) with EMCCD observations. Astronomy and Astrophysics, 592, [A120]. https://doi.org/10.1051/0004-6361/201628864 Published in: Astronomy and Astrophysics Citing this paper Please note that where the full-text provided on Manchester Research Explorer is the Author Accepted Manuscript or Proof version this may differ from the final Published version. If citing, it is advised that you check and use the publisher's definitive version. General rights Copyright and moral rights for the publications made accessible in the Research Explorer are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. Takedown policy If you believe that this document breaches copyright please refer to the University of Manchester’s Takedown Procedures [http://man.ac.uk/04Y6Bo] or contact [email protected] providing relevant details, so we can investigate your claim. -
2020-21 LSU Research Magazine, Frontiers
Office of Research & Economic Development ···························· The Constant Pursuit of Discovery | 2020-21 TABLE OF CONTENTS 8 CORONAVIRUS 26 BLACK HOLE 18 EXPEDITION 32 CARBON 22 FOUNTAIN OF YOUTH News Scholarship Recognition 3 Briefs 36 Black and Essential 48 Rainmakers 6 Q&A 40 Feltus Taylor 51 Accolades 45 Microbes 57 Distinguished Research Masters 59 Media Shelf NEWS BRIEFS ABOUT THIS ISSUE LSU Research is published annually by the Office of NEWS Research & Economic Development, Louisiana State University, with editorial offices in 134 David F. Boyd Hall, LSU, Baton Rouge, LA 70803. Any written portion of this Newly Discovered Mineral Named Tracking the Dangers of Vaping publication may be reprinted without permission as long as credit for LSU Research is given. Opinions expressed for LSU Geologist By Sandra Sarr herein do not necessarily reflect those of LSU faculty or administration. By Jonathan Snow When electronic cigarettes made their debut on the market Send correspondence to the Office of Research & Like stars and ships, it is rare about 10 years ago, the general public believed they offered Economic Development at the address above or email a harmless alternative to cigarette smoking. However, that [email protected], call 225-578-5833, and visit us at: for a new mineral to be named lsu.edu/research. For more great research stories, visit: after a living person. However, notion has gone up in smoke as evidence of harmful health lsu.edu/research/news. that honor was accorded effects builds. As of December 2019, more than 2,561 people throughout the U.S. have been hospitalized or died due to lung Louisiana State University and Office of Research to LSU mineralogist Barb & Economic Development Administration Dutrow by the International injuries linked to vaping or e-cigarette use, according to the FROM THE Thomas Galligan, Interim President Mineralogical Association. -
New Type of Black Hole Detected in Massive Collision That Sent Gravitational Waves with a 'Bang'
New type of black hole detected in massive collision that sent gravitational waves with a 'bang' By Ashley Strickland, CNN Updated 1200 GMT (2000 HKT) September 2, 2020 <img alt="Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image." class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190516104725-ngc-4485-nasa-super-169.jpg"> Photos: Wonders of the universe Galaxy NGC 4485 collided with its larger galactic neighbor NGC 4490 millions of years ago, leading to the creation of new stars seen in the right side of the image. Hide Caption 98 of 195 <img alt="Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. " class="media__image" src="//cdn.cnn.com/cnnnext/dam/assets/190502151952-0502-wonders-of-the-universe-super-169.jpg"> Photos: Wonders of the universe Astronomers developed a mosaic of the distant universe, called the Hubble Legacy Field, that documents 16 years of observations from the Hubble Space Telescope. The image contains 200,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the Big Bang. Hide Caption 99 of 195 <img alt="A ground-based telescope&amp;#39;s view of the Large Magellanic Cloud, a neighboring galaxy of our Milky Way.