Crystal Clue to Quantum Gravity
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Cosmicflows-3: Cosmography of the Local Void
Draft version May 22, 2019 Preprint typeset using LATEX style AASTeX6 v. 1.0 COSMICFLOWS-3: COSMOGRAPHY OF THE LOCAL VOID R. Brent Tully, Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA Daniel Pomarede` Institut de Recherche sur les Lois Fondamentales de l'Univers, CEA, Universite' Paris-Saclay, 91191 Gif-sur-Yvette, France Romain Graziani University of Lyon, UCB Lyon 1, CNRS/IN2P3, IPN Lyon, France Hel´ ene` M. Courtois University of Lyon, UCB Lyon 1, CNRS/IN2P3, IPN Lyon, France Yehuda Hoffman Racah Institute of Physics, Hebrew University, Jerusalem, 91904 Israel Edward J. Shaya University of Maryland, Astronomy Department, College Park, MD 20743, USA ABSTRACT Cosmicflows-3 distances and inferred peculiar velocities of galaxies have permitted the reconstruction of the structure of over and under densities within the volume extending to 0:05c. This study focuses on the under dense regions, particularly the Local Void that lies largely in the zone of obscuration and consequently has received limited attention. Major over dense structures that bound the Local Void are the Perseus-Pisces and Norma-Pavo-Indus filaments sepa- rated by 8,500 km s−1. The void network of the universe is interconnected and void passages are found from the Local Void to the adjacent very large Hercules and Sculptor voids. Minor filaments course through voids. A particularly interesting example connects the Virgo and Perseus clusters, with several substantial galaxies found along the chain in the depths of the Local Void. The Local Void has a substantial dynamical effect, causing a deviant motion of the Local Group of 200 − 250 km s−1. -
Jul/Aug 2013
I NTERNATIONAL J OURNAL OF H IGH -E NERGY P HYSICS CERNCOURIER WELCOME V OLUME 5 3 N UMBER 6 J ULY /A UGUST 2 0 1 3 CERN Courier – digital edition Welcome to the digital edition of the July/August 2013 issue of CERN Courier. This “double issue” provides plenty to read during what is for many people the holiday season. The feature articles illustrate well the breadth of modern IceCube brings particle physics – from the Standard Model, which is still being tested in the analysis of data from Fermilab’s Tevatron, to the tantalizing hints of news from the deep extraterrestrial neutrinos from the IceCube Observatory at the South Pole. A connection of a different kind between space and particle physics emerges in the interview with the astronaut who started his postgraduate life at CERN, while connections between particle physics and everyday life come into focus in the application of particle detectors to the diagnosis of breast cancer. And if this is not enough, take a look at Summer Bookshelf, with its selection of suggestions for more relaxed reading. To sign up to the new issue alert, please visit: http://cerncourier.com/cws/sign-up. To subscribe to the magazine, the e-mail new-issue alert, please visit: http://cerncourier.com/cws/how-to-subscribe. ISOLDE OUTREACH TEVATRON From new magic LHC tourist trail to the rarest of gets off to a LEGACY EDITOR: CHRISTINE SUTTON, CERN elements great start Results continue DIGITAL EDITION CREATED BY JESSE KARJALAINEN/IOP PUBLISHING, UK p6 p43 to excite p17 CERNCOURIER www. -
The Standard Model
The Standard Model by Christine Sutton In May 1983, the central detector of the UA1 experiment at CERN's proton-antiproton collider showed the tell-tale signature of the long-awaited Z particle as it decays into an electron-positron pair (arrowed). As the electrically neutral carrier of the weak force, the Z° plays a vital role in the Standard Model. The initial evidence from Fermilab (see previous article) for the long awaited sixth ('top') quark puts another rivet in the already firm structure of today's Standard Model of physics. Analysis of the Fermilab CDF data gives a top mass of 174 GeV with an error of ten per cent either way. This falls within the mass band predicted by the sum total of world Standard Model data and underlines our understanding of physics in terms of six quarks and six leptons. Model encompasses all the elemen their interactions emerge. Instead it is In this specially commissioned tary particles we now know and three an amalgam of the best theories we overview, physics writer Christine of the fundamental forces. The basic have, which we can bolt together Sutton explains the Standard building blocks are two sets or because they have enough in com Model. "families" or "matter particles" - the mon to suggest an underlying unity, quarks and the leptons (see page 5). although due to our ignorance the These particles interact with each joins still clearly show. t is nearly 100 years since the other through the exchange of force The structure as a whole rests on a I discovery of the first subatomic carriers or "messengers". -
Observing List
day month year Epoch 2000 local clock time: 23.98 Observing List for 23 7 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 20 50 Andromeda Gamma Andromedae (*266) 2.3 5.5 9.8 yellow & blue green double star 2 3.9 42 19 28 69 Andromeda Pi Andromedae 4.4 8.6 35.9 bright white & faint blue 0 36.9 33 43 30 55 Andromeda STF 79 (Struve) 6 7 7.8 bluish pair 1 0.1 44 42 16 52 Andromeda 59 Andromedae 6.5 7 16.6 neat pair, both greenish blue 2 10.9 39 2 45 67 Andromeda NGC 7662 (The Blue Snowball) planetary nebula, fairly bright & slightly elongated 23 25.9 42 32.1 31 60 Andromeda M31 (Andromeda Galaxy) large sprial arm galaxy like the Milky Way 0 42.7 41 16 31 61 Andromeda M32 satellite galaxy of Andromeda Galaxy 0 42.7 40 52 32 60 Andromeda M110 (NGC205) satellite galaxy of Andromeda Galaxy 0 40.4 41 41 17 55 Andromeda NGC752 large open cluster of 60 stars 1 57.8 37 41 17 48 Andromeda NGC891 edge on galaxy, needle-like in appearance 2 22.6 42 21 45 69 Andromeda NGC7640 elongated galaxy with mottled halo 23 22.1 40 51 46 57 Andromeda NGC7686 open cluster of 20 stars 23 30.2 49 8 30 121 Aquarius 55 Aquarii, Zeta 4.3 4.5 2.1 close, elegant pair of yellow stars 22 28.8 0 -1 12 120 Aquarius 94 Aquarii 5.3 7.3 12.7 pale rose & emerald 23 19.1 -13 28 32 152 Aquarius M72 globular cluster 20 53.5 -12 32 31 151 Aquarius M73 Y-shaped asterism of 4 stars 20 59 -12 38 16 117 Aquarius NGC7606 Galaxy 23 19.1 -8 29 32 149 Aquarius NGC7009 Saturn Neb planetary nebula, large & bright pale green oval 21 4.2 -11 21.8 38 135 -
And Ecclesiastical Cosmology
GSJ: VOLUME 6, ISSUE 3, MARCH 2018 101 GSJ: Volume 6, Issue 3, March 2018, Online: ISSN 2320-9186 www.globalscientificjournal.com DEMOLITION HUBBLE'S LAW, BIG BANG THE BASIS OF "MODERN" AND ECCLESIASTICAL COSMOLOGY Author: Weitter Duckss (Slavko Sedic) Zadar Croatia Pусскй Croatian „If two objects are represented by ball bearings and space-time by the stretching of a rubber sheet, the Doppler effect is caused by the rolling of ball bearings over the rubber sheet in order to achieve a particular motion. A cosmological red shift occurs when ball bearings get stuck on the sheet, which is stretched.“ Wikipedia OK, let's check that on our local group of galaxies (the table from my article „Where did the blue spectral shift inside the universe come from?“) galaxies, local groups Redshift km/s Blueshift km/s Sextans B (4.44 ± 0.23 Mly) 300 ± 0 Sextans A 324 ± 2 NGC 3109 403 ± 1 Tucana Dwarf 130 ± ? Leo I 285 ± 2 NGC 6822 -57 ± 2 Andromeda Galaxy -301 ± 1 Leo II (about 690,000 ly) 79 ± 1 Phoenix Dwarf 60 ± 30 SagDIG -79 ± 1 Aquarius Dwarf -141 ± 2 Wolf–Lundmark–Melotte -122 ± 2 Pisces Dwarf -287 ± 0 Antlia Dwarf 362 ± 0 Leo A 0.000067 (z) Pegasus Dwarf Spheroidal -354 ± 3 IC 10 -348 ± 1 NGC 185 -202 ± 3 Canes Venatici I ~ 31 GSJ© 2018 www.globalscientificjournal.com GSJ: VOLUME 6, ISSUE 3, MARCH 2018 102 Andromeda III -351 ± 9 Andromeda II -188 ± 3 Triangulum Galaxy -179 ± 3 Messier 110 -241 ± 3 NGC 147 (2.53 ± 0.11 Mly) -193 ± 3 Small Magellanic Cloud 0.000527 Large Magellanic Cloud - - M32 -200 ± 6 NGC 205 -241 ± 3 IC 1613 -234 ± 1 Carina Dwarf 230 ± 60 Sextans Dwarf 224 ± 2 Ursa Minor Dwarf (200 ± 30 kly) -247 ± 1 Draco Dwarf -292 ± 21 Cassiopeia Dwarf -307 ± 2 Ursa Major II Dwarf - 116 Leo IV 130 Leo V ( 585 kly) 173 Leo T -60 Bootes II -120 Pegasus Dwarf -183 ± 0 Sculptor Dwarf 110 ± 1 Etc. -
From Messier to Abell: 200 Years of Science with Galaxy Clusters
Constructing the Universe with Clusters of Galaxies, IAP 2000 meeting, Paris (France) July 2000 Florence Durret & Daniel Gerbal eds. FROM MESSIER TO ABELL: 200 YEARS OF SCIENCE WITH GALAXY CLUSTERS Andrea BIVIANO Osservatorio Astronomico di Trieste via G.B. Tiepolo 11 – I-34131 Trieste, Italy [email protected] 1 Introduction The history of the scientific investigation of galaxy clusters starts with the XVIII century, when Charles Messier and F. Wilhelm Herschel independently produced the first catalogues of nebulæ, and noticed remarkable concentrations of nebulæ on the sky. Many astronomers of the XIX and early XX century investigated the distribution of nebulæ in order to understand their relation to the local “sidereal system”, the Milky Way. The question they were trying to answer was whether or not the nebulæ are external to our own galaxy. The answer came at the beginning of the XX century, mainly through the works of V.M. Slipher and E. Hubble (see, e.g., Smith424). The extragalactic nature of nebulæ being established, astronomers started to consider clus- ters of galaxies as physical systems. The issue of how clusters form attracted the attention of K. Lundmark287 as early as in 1927. Six years later, F. Zwicky512 first estimated the mass of a galaxy cluster, thus establishing the need for dark matter. The role of clusters as laboratories for studying the evolution of galaxies was also soon realized (notably with the collisional stripping theory of Spitzer & Baade430). In the 50’s the investigation of galaxy clusters started to cover all aspects, from the distri- bution and properties of galaxies in clusters, to the existence of sub- and super-clustering, from the origin and evolution of clusters, to their dynamical status, and the nature of dark matter (or “positive energy”, see e.g., Ambartsumian29). -
The Challenge of Neutrinos by Christine Sutton
The challenge of neutrinos by Christine Sutton Neutrino pioneers - left to right, Paul Dirac, Wolfgang Pauli., Rudolf Peierls. (Photo MP Niels Bohr Library) Earlier this year, a team of physicists working at Los Alamos claimed a possible sighting of neutrino oscillations (June, page 13). However even before the claim appeared in the scientific literature, newspaper reports had leaked the possible findings and their implications. Detecting particles which can pass unhindered through the Earth provides the ultimate physics challenge. Neutrinos have always captivated public imagination and make compelling reading. In the wake of the latest neutrino episode, Oxford physi cist and science writer Christine Sutton looks back on the short but volatile history of the neutrino and its attendant publicity. strangers to controversy, for they beta-decay electrons varies continu With the availability of high were in a sense born amidst it, and ously up to a maximum, with peaks energy neutrino beams in the as recent work on neutrino oscilla ("lines") at only a few energies. And 1970s, physicists eagerly tions demonstrates they continue to he was able to explain how the scoured each new batch of data fuel debate. This is of course largely photographic technique could "fake" for signs of exciting new physics. to do with the fact that neutrinos have lines through its great sensitivity to But few initial 'sightings' proved no electric charge and experience small changes in intensity. to be of substance. One of the only the weak nuclear force, making The First World War interrupted major problems faced by such them supremely difficult to detect. -
Taking the Subatomic Grand Tour the Secrets of the World of Elementary Particles Revealed
book reviews Taking the subatomic Grand Tour The secrets of the world of elementary particles revealed. The Particle Odyssey: A Journey to the Heart of Matter by Frank Close, Michael Marten & FERMILAB Christine Sutton Oxford University Press: 2002. 246 pp. £29.95, $45. Ken Peach The development of the standard model of particles and their interactions is one of the major scientific achievements of the twen- tieth century. The electron was the first ‘elementary particle’ to be discovered, by J. J. Thomson (working largely on his own) in 1897, and the top quark was the last of the standard model’s ‘fundamental fermions’ to be discovered, by two large teams at the Tevatron near Chicago in 1995. In between, special and general relativity, quantum mechanics and a deep understanding of symmetry (explicit and hidden, global and local, absolute and spontaneously broken) have transformed our understanding of the dynamics of the Universe. Within this frame- work, a remarkably complete description of the way in which the Universe works has Problem particle: the top quark, here decaying into muons (blue tracks), wasn’t discovered until 1995. been developed, and all but one of its ingre- dients experimentally verified — only the ingredient (quarks, leptons, gauge bosons tions. Most of the loopholes have since been elusive Higgs particle remains undetected. and other whimsies associated with high- closed: the top quark has now been discov- The Particle Odyssey describes a century energy physics) is described and illustrated, ered, the electroweak sector has survived of discovery and creativity through a series along with photographs and biographical precision scrutiny at the Large Electron– of stunning images and photographs. -
The Galaxies of Serpens Caput by Mark Bratton, Montreal Centre ([email protected])
Scenic Vistas The Galaxies of Serpens Caput by Mark Bratton, Montreal Centre ([email protected]) xcept for the relative minority of Located on a line amateur astronomers who conduct joining beta and delta Esystematic scientific research with Serpentis, NGC 5970 is their telescopes, most of us are very much one of the brightest tourists in our approach to the universe. galaxies this region has We set up our instruments when our busy to offer. Located about schedules permit and are very much at eight arcminutes the mercies of the fickle nature of the southwest of a weather in these parts. Our time at the magnitude +8 field star, telescope is precious and we try not to this spiral galaxy is waste too much of it in fruitless pursuit oriented due east/west of unattainable objects. So we often stick and features a very to the tried and true, best exemplified by bright and small core the entries on the Messier list. embedded in a bright One of the reasons why I started bar oriented along the writing this column seven years ago was major axis. In my 15-inch my intention was to draw attention to reflector, this bar ap- interesting sights in the universe that pears quite mottled, would otherwise not be well-known. In and one’s attention is travel guides for tourists here on Earth, drawn to a brighter breathtaking scenery is often referred to condensation im- An ~8-arcminute Digitized Sky Survey1 field of Seyfert’s Sextet, a faint as a scenic vista, hence the name of this mediately east of the group of galaxies in Serpens Caput. -
The Great Survivor
Dubna - the great survivor atoms are now around the corner. This year, as CERN celebrates its chine in the world. This machine is The Conference closed with the 40th anniversary (November, page still operational, and features in the award of N. Hamann Prize to A. 26), not far behind in the celebration Guinness Book of records as the Masoni of Cagliari, for his presenta stakes is the Joint Institute for Nu planet's largest electromagnet. tion on a high statistics study of iota clear Research, Dubna, near Mos While eclipsed by the new genera decay with the Obelix spectrometer. cow, established in 1956. While tion of strong focusing machines, the This Prize, funded by the Jozef CERN's goal was to provide a Synchrophasotron enjoyed a new Stefan Institute, Ljubljana, is in physics platform on which to rebuild lease of life as a heavy ion machine memory of Niklaus Hamann, PS Western European science after (up to silicon-28), as well as provid coordinator and LEAR physicist who World War II, JINR had a similar ing polarized deuteron beams. The died last year, aged 40. mission for the USSR and the social machine currently runs for some ist countries, including Eastern 1,500 hours per year, providing Europe. research material for more than 500 The fact that both organizations are scientists from 100 institutions. reaching their 40th anniversary The next energy step had very testifies to their success. While their different scenarios at CERN and at aims were very similar, their political JINR. In in the early 1970s, CERN contexts and scientific strategies decided to build the '300 GeV have led along very different routes. -
Thirty Years of Erice on the Brane1
IMPERIAL-TP-2018-MJD-03 Thirty years of Erice on the brane1 M. J. Duff Institute for Quantum Science and Engineering and Hagler Institute for Advanced Study, Texas A&M University, College Station, TX, 77840, USA & Theoretical Physics, Blackett Laboratory, Imperial College London, London SW7 2AZ, United Kingdom & Mathematical Institute, Andrew Wiles Building, University of Oxford, Oxford OX2 6GG, United Kingdom Abstract After initially meeting with fierce resistance, branes, p-dimensional extended objects which go beyond particles (p = 0) and strings (p = 1), now occupy centre stage in the- oretical physics as microscopic components of M-theory, as the seeds of the AdS/CFT correspondence, as a branch of particle phenomenology, as the higher-dimensional pro- arXiv:1812.11658v2 [hep-th] 16 Jun 2019 genitors of black holes and, via the brane-world, as entire universes in their own right. Notwithstanding this early opposition, Nino Zichichi invited me to to talk about su- permembranes and eleven dimensions at the 1987 School on Subnuclear Physics and has continued to keep Erice on the brane ever since. Here I provide a distillation of my Erice brane lectures and some personal recollections. 1Based on lectures at the International Schools of Subnuclear Physics 1987-2017 and the International Symposium 60 Years of Subnuclear Physics at Bologna, University of Bologna, November 2018. Contents 1 Introduction 5 1.1 Geneva and Erice: a tale of two cities . 5 1.2 Co-authors . 9 1.3 Nomenclature . 9 2 1987 Not the Standard Superstring Review 10 2.1 Vacuum degeneracy and the multiverse . 11 2.2 Supermembranes . -
CERN Courier April 2014 Viewpoint Cividec Instrumentation
CERN Courier April 2014 Viewpoint cividec Instrumentation CIVIDEC Instrumentation is a R&D company born from the cutting-edge technology of CERN. We specialise in turn-key The 1980s: spurring collaboration solutions for beam diagnostics based on CVD diamond technology. Herwig Schopper recalls a transferred to new assignments. Another element of “anti-growth” had decade of growth at CERN. long-term consequences. Council was Diamond Detectors convinced that the scientifi c programme was fi rst class, but had doubts about the effi ciency of management. An evaluation committee The 1980s were characterized was established to assess the human and by two outstanding material resources, with a view to reducing achievements that were to the CERN budget. In the end, the committee infl uence the long-term declined to consider a lower material future of CERN. First came the discovery budget because this would undoubtedly of the W and Z particles, the carriers of the jeopardize the excellent scientifi c record of weak force, produced in proton–antiproton Herwig Schopper in 1982: with LEP a “new CERN. They proposed instead a reduction collisions at the Super Proton Synchrotron ‘sociology’ for international scientifi c of staff from about 3500 to 2500, through (SPS) and detected by the UA1 and UA2 co-operation was born”. (Image credit: an early retirement programme, and during experiments. These were the fi rst, now-typical CERN-PHOTO-8205525.) the construction of the LHC this was even collider experiments, covering the full lowered to 2000. However, to cope with solid angle and requiring large groups the time with Israel and Turkey failed, for the increasing tasks and the rising number of collaborators from many countries.