Early Photons from the Early Universe
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Far Side of the Moore by Sean Grundy
Far Side Of The Moore By Sean Grundy CHARACTERS PATRICK MOORE (early 30s)...eccentric amateur astronomer PAUL JOHNSTONE (mid 30s)...BBC science producer DR HENRY KING (40s) ...soon-to-be head of the BAA PERCY WILKINS (60s) ...Moore’s mentor EILEEN WILKINS (early 20s) ...Percy’s daughter ARTHUR C CLARKE (late 30s)...Moore’s friend GERTRUDE MOORE (60s)...Moore’s mother LEONARD MIALL (40s)...BBC Head of Talks ANNOUNCER; STUDIO FM; TRANSMISSION CONTROL; HENRY KING’S SECRETARY; NEWS REPORTER; GEORGE ADAMSKI; BAA PRESIDENT Set in mid-1950s at BBC TV, BAA meeting room and Patrick’s home, East Grinstead. (Draft 4 - 27/01/15) SCENE 1.INTRO. SFX SPACEY FX/MUSIC ANNOUNCER The following drama is based on the true story of Patrick Moore and the making of ‘The Sky At Night’. PATRICK MOORE (OLDER) All true, even the stuff I exaggerated to jolly up the proceedings. However, I do apologise for my restraint on more colourful opinions: PC-brigade, female producers, Europhiles and all that. Damn irritating.. (FADE) SFX SPACEY MUSIC – MIX TO – RADIO DIAL REWINDING BACK IN TIME TO: SCENE 2.INT. BBC STUDIO. 1957 ARCHIVE (OR MOCK-UP) CYRIL STAPLETON’S PARADE MUSIC PLAYS PAUL JOHNSTONE ..Countdown to live in 90..Ident, please.. STUDIO FM (ON TALKBACK) Sky At Night. Programme 1. 24/4/57. 10.30pm. Transmission, do you have a feed? TRANSMISSION CONTROL (ON TALKBACK) Hello, studio. Rolling credits on ‘Cyril Stapleton Parade’. I see your slate: (READS) ‘Producer, Paul Johnstone. Host, Patrick Meere.’ STUDIO FM (ON TALKBACK) ‘Moore’. TRANSMISSION CONTROL Correction, ‘Moore’. STUDIO FM (ON TALKBACK) Live in 60. -
Leed® Gold Certification
MADONNA NOW The Magazine of Madonna University PRESIDENT’S REPORT 2010 ER D C TIF EE IE L D Cover Story LEED® GOLD CERTIFICATION Awarded to Madonna’s Franciscan Center GOLD ALUMNI MADONNA UNIVERSITY MADONNA UNIVERSITY 36600 Schoolcraft Road OF CONTENTS TABLE CENTER Livonia, MI 48150-1176 Admissions Office Welcome 734-432-5339 Alumni & Friends! ALUMNI Advancement Office Take advantage of all 41 734-432-5589 Madonna University offers Alumni Office its alumni. Whether you 734-432-5811 want to stay connected by updating your contact info, Main Number TASSEL 734-432-5300 or purchase a spirit tassel or 800-852-4951 brick paver, or volunteer to Spirit help with a Madonna event, [email protected] we’d love to see you. Next www.madonna.edu time you’re in the area, drop The spirit tassel symbolizes in and learn about these and support of the mission and values Editorial Staff The Madonna Now is published by other alumni benefits: of Madonna University. Make a 12 6 the Office of University Advancement Spirit Tassel Gift to the Annual Graduate School tuition Andrea Nodge ’84 discount Fund in the amount of your class vice president for advancement 2 Library & Computer Lab use year and receive this keepsake as President’s Perspective Living our Mission Karen Sanborn Job listings and career a reminder of your educational director of marketing assistance journey at Madonna. 5 Campus Living is Easy Decking the Halls Jill N. Hamilton-Krawczyk ’08 Alumni Scholarship for your graphic designer children 6 Fransciscan Center Awarded Gold To make your gift, contact LEED® Gold Certification Alan Piñon ’03 Access to alumni in the Amy Perry, alumni relations officer, marketing officer U.S. -
People and Things
People and things Geoff Manning for his contributions Dirac Medal to physics applications at the Lab oratory, particularly in high energy At the recent symposium on 'Per physics, computing and the new spectives in Particle Physics' at Spallation Neutron Source. The the International Centre for Theo Rutherford Prize goes to Alan Ast- retical Physics, Trieste, ICTP Direc bury of Victoria, Canada, former tor Abdus Sa la m presided over co-spokesman of the UA 1 experi the first award ceremony for the ment at CERN. Institute's Dirac Medals. Although Philip Anderson (Princeton) and expected, Yakov Zeldovich of Abdus Sa la m (Imperial College Moscow's Institute of Space Re London and the International search was not able to attend to Centre for Theoretical Physics, receive his medal. Edward Witten Trieste) have been elected Hono of Princeton received his gold me rary Fellows of the Institute. dal alone from Antonino Zichichi on behalf of the Award Committee. Third World Prizes The 1985 Third World Academy UK Institute of Physics Awards of Sciences Physics Prize has been awarded to E. C. G. Sudarshan The Guthrie Prize and Medal of the from India for his fundamental con UK Institute of Physics this year tributions to the understanding of goes to Sir Denys Wilkinson of the weak nuclear force, in particu Sussex for his many contributions lar for his work with R. Marshak to nuclear physics. The Institute's on the theory which incorporates Glazebrook Prize goes to Ruther its parity (left/right symmetry) Friends and colleagues recently ford Appleton Laboratory director structure. -
Cosmic Background Explorer (COBE) and Beyond
From the Big Bang to the Nobel Prize: Cosmic Background Explorer (COBE) and Beyond Goddard Space Flight Center Lecture John Mather Nov. 21, 2006 Astronomical Search For Origins First Galaxies Big Bang Life Galaxies Evolve Planets Stars Looking Back in Time Measuring Distance This technique enables measurement of enormous distances Astronomer's Toolbox #2: Doppler Shift - Light Atoms emit light at discrete wavelengths that can be seen with a spectroscope This “line spectrum” identifies the atom and its velocity Galaxies attract each other, so the expansion should be slowing down -- Right?? To tell, we need to compare the velocity we measure on nearby galaxies to ones at very high redshift. In other words, we need to extend Hubble’s velocity vs distance plot to much greater distances. Nobel Prize Press Release The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics for 2006 jointly to John C. Mather, NASA Goddard Space Flight Center, Greenbelt, MD, USA, and George F. Smoot, University of California, Berkeley, CA, USA "for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation". The Power of Thought Georges Lemaitre & Albert Einstein George Gamow Robert Herman & Ralph Alpher Rashid Sunyaev Jim Peebles Power of Hardware - CMB Spectrum Paul Richards Mike Werner David Woody Frank Low Herb Gush Rai Weiss Brief COBE History • 1965, CMB announced - Penzias & Wilson; Dicke, Peebles, Roll, & Wilkinson • 1974, NASA AO for Explorers: ~ 150 proposals, including: – JPL anisotropy proposal (Gulkis, Janssen…) – Berkeley anisotropy proposal (Alvarez, Smoot…) – Goddard/MIT/Princeton COBE proposal (Hauser, Mather, Muehlner, Silverberg, Thaddeus, Weiss, Wilkinson) COBE History (2) • 1976, Mission Definition Science Team selected by HQ (Nancy Boggess, Program Scientist); PI’s chosen • ~ 1979, decision to build COBE in-house at GSFC • 1982, approval to construct for flight • 1986, Challenger explosion, start COBE redesign for Delta launch • 1989, Nov. -
Cities and Their Vital Systems: Infrastructure Past, Present, and Future
Cities and Their Vital Systems: Infrastructure Past, Present, and Future i Series on Technology and Social Priorities NATIONAL ACADEMY OF ENGINEERING CitiesCitiesCities andandand TheirTheirTheir VitalVitalVital SystemsSystemsSystems Infrastructure Past, Present, and Future Jesse H. Ausubel and Robert Herman Editors NATIONAL ACADEMY PRESS Washington, D.C. 1988 Copyright National Academy of Sciences. All rights reserved. Cities and Their Vital Systems: Infrastructure Past, Present, and Future ii National Academy Press 2101 Constitution Avenue, NW Washington, DC 20418 NOTICE: The National Academy of Engineering was established in 1964, under the charter of the National Academy of Sciences, as a parallel organization of outstanding engineers. It is autonomous in its administration and in the selection of its members, sharing with the National Academy of Sci- ences the responsibility for advising the federal government. The National Academy of Engineering also sponsors engineering programs aimed at meeting national needs, encourages education and research, and recognizes the superior achievement of engineers. Dr. Robert M. White is president of the National Academy of Engineering. Funds for the National Academy of Engineering's Symposium Series on Technology and Social Priorities were provided by the Andrew W. Mellon Foundation, Carnegie Corporation of New York, and the Academy's Technology Agenda Program. This publication has been reviewed by a group other than the authors according to procedures approved by a Report Review Committee. The views expressed in this volume are those of the authors and are not presented as the views of the Mellon Foundation, Carnegie Corporation, or the National Academy of Engineering. Library of Congress Cataloging-in-Publication Data Cities and their vital systems. -
Annual Report 2016 ↓ Section 0 2 — School Council
ANNUAL REPORT 2016 ↓ SECTION SECTION 0 2 — SCHOOL COUNCIL SCHOOL Geelong Grammar School Corio Campus 50 Biddlecombe Avenue Corio, Victoria 3214 T +61 3 5273 9231 F +61 3 5273 9356 www.ggs.vic.edu.au CRICOS 00143G ABN 92 004 971 500 2 ANNUAL REPORT 2016 - GEELONG GRAMMAR SCHOOL ↓ CONTENTS SECTION 0 2 — SCHOOL COUNCIL SCHOOL 04 12 33 COUNCIL REPORT FOUNDATION REPORT OGG REPORT Jeremy Kirkwood (FB’79) Penny McBain Margie Gillett (Cordner, Cl’71) 08 16 35 COUNCIL FOUNDATION OGG FINANCIAL SUMMARY FINANCIAL SUMMARY FINANCIAL SUMMARY 10 22 34 COUNCIL FOUNDATION OGG MEMBERS BOARD COMMITTEE 25 FOUNDATION MEMBERS 29 FOUNDATION DONORS ANNUAL REPORT 2016 - GEELONG GRAMMAR SCHOOL 3 ↓ SECTION SECTION 0 2 — SCHOOL COUNCIL SCHOOL COUNCIL REPORT I AM PLEASED TO PRESENT THE CHAIRMAN’S REPORT FOR 2016 TOGETHER WITH THE ABRIDGED 2016 FINANCIAL ACCOUNTS. 2016 was a consolidating year after the School’s appearance before the Royal Commission into Institutional Responses to Child Sexual Abuse in September and October 2015. The School established a Recognition Committee following the Royal Commission’s public hearings, which met three times in 2016. The School implemented the major recommendation of the Recognition Committee by appointing a Survivor Liaison Coordinator, Renee Handsaker, to provide outreach and support to survivors of child sexual abuse at the School. Ms Handsaker has performed a vital role assisting survivors in a confidential and independent way. Her role is complimentary to, but separate of, the independent counsellor provided by the School to offer counselling and advice. The Royal Commission released its final report from the School’s case study in February 2017. -
Hawking Radiation and the Expansion of the Universe
Hawking radiation and the expansion of the universe 1 2, 3 Yoav Weinstein , Eran Sinbar *, and Gabriel Sinbar 1 DIR Technologies, Matam Towers 3, 6F, P.O.Box 15129, Haifa, 319050, Israel 2 DIR Technologies, Matam Towers 3, 6F, P.O.Box 15129, Haifa, 3190501, Israel 3 RAFAEL advanced defense systems ltd., POB 2250(19), Haifa, 3102102, Israel * Corresponding author: Eran Sinbar, Ela 13, Shorashim, Misgav, 2016400, Israel, Telephone: +972-4-9028428, Mobile phone: +972-523-713024, Email: [email protected] ABSTRUCT Based on Heisenberg’s uncertainty principle it is concluded that the vacuum is filed with matter and anti-matter virtual pairs (“quantum foam”) that pop out and annihilate back in a very short period of time. When this quantum effects happen just outside the "event horizon" of a black hole, there is a chance that one of these virtual particles will pass through the event horizon and be sucked forever into the black hole while its partner virtual particle remains outside the event horizon free to float in space as a real particle (Hawking Radiation). In our previous work [1], we claim that antimatter particle has anti-gravity characteristic, therefore, we claim that during the Hawking radiation procedure, virtual matter particles have much larger chance to be sucked by gravity into the black hole then its copartner the anti-matter (anti-gravity) virtual particle. This leads us to the conclusion that hawking radiation is a significant source for continuous generation of mostly new anti-matter particles, spread in deep space, contributing to the expansion of space through their anti-gravity characteristic. -
Patrick Moore's Practical Astronomy Series
Patrick Moore’s Practical Astronomy Series Other Titles in this Series Navigating the Night Sky Astronomy of the Milky Way How to Identify the Stars and The Observer’s Guide to the Constellations Southern/Northern Sky Parts 1 and 2 Guilherme de Almeida hardcover set Observing and Measuring Visual Mike Inglis Double Stars Astronomy of the Milky Way Bob Argyle (Ed.) Part 1: Observer’s Guide to the Observing Meteors, Comets, Supernovae Northern Sky and other transient Phenomena Mike Inglis Neil Bone Astronomy of the Milky Way Human Vision and The Night Sky Part 2: Observer’s Guide to the How to Improve Your Observing Skills Southern Sky Michael P. Borgia Mike Inglis How to Photograph the Moon and Planets Observing Comets with Your Digital Camera Nick James and Gerald North Tony Buick Telescopes and Techniques Practical Astrophotography An Introduction to Practical Astronomy Jeffrey R. Charles Chris Kitchin Pattern Asterisms Seeing Stars A New Way to Chart the Stars The Night Sky Through Small Telescopes John Chiravalle Chris Kitchin and Robert W. Forrest Deep Sky Observing Photo-guide to the Constellations The Astronomical Tourist A Self-Teaching Guide to Finding Your Steve R. Coe Way Around the Heavens Chris Kitchin Visual Astronomy in the Suburbs A Guide to Spectacular Viewing Solar Observing Techniques Antony Cooke Chris Kitchin Visual Astronomy Under Dark Skies How to Observe the Sun Safely A New Approach to Observing Deep Space Lee Macdonald Antony Cooke The Sun in Eclipse Real Astronomy with Small Telescopes Sir Patrick Moore and Michael Maunder Step-by-Step Activities for Discovery Transit Michael K. -
The Big Bang
15- THE BIG ORIGINS BANGANAND NARAYANAN The Big Bang theory “Who really knows, who can declare? The scientific study of the origin and currently occupies When it started or where from? evolution of the universe is called the center stage in From when and where this creation has arisen cosmology. From the early years of the modern cosmology. 20th century, the observational aspects Perhaps it formed itself, perhaps it did not.” And yet, half a of scientific cosmology began to gather century ago, it was – Rig Veda (10:129), 9th century BCE. wide attention. This was because of only one among a a small series of startling discoveries few divergent world made by scientists like Edwin Hubble views, with competing hese words were written over 2000 years that changed the way we understood claims to the truth. ago. And yet, if they sound contemporary, it the physical universe. This article highlights Tis because they echo a trait that is distinctly a few trail-blazing human; the highly evolved ability of our species to Hubble had an advantage which few events in the journey look at the world around us and wonder how it all astronomers in the early 20th century of the Big Bang model came to be. How often have you asked these very had – access to the Mount Wilson from the fringes to same questions? Observatory in California. This the centerfold of particular observatory housed the astrophysics, a We assume that all things have a beginning. Could this be true for this vastly complex universe as well? largest telescopes of that time and journey that is yielded high quality data. -
Frequency of Hawking Radiation of Black Holes
International Journal of Astrophysics and Space Science 2013; 1(4): 45-51 Published online October 30, 2013 (http://www.sciencepublishinggroup.com/j/ijass) doi: 10.11648/j.ijass.20130104.15 Frequency of Hawking radiation of black holes Dipo Mahto 1, Brajesh Kumar Jha 2, Krishna Murari Singh 1, Kamala Parhi 3 1Dept. of Physics, Marwari College, T.M.B.U. Bhagalpur-812007, India 2Deptartment of Physics, L.N.M.U. Darbhanga, India 3Dept. of Mathematics, Marwari College, T.M.B.U. Bhagalpur-812007, India Email address: [email protected](D. Mahto), [email protected](B. K. Jha), [email protected](K. M. Singh), [email protected] (K . Parhi) To cite this article: Dipo Mahto, Brajesh Kumar Jha, Krishna Murari Singh, Kamala Parhi. Frequency of Hawking Radiation of Black Holes. International Journal of Astrophysics and Space Science. Vol. 1, No. 4, 2013, pp. 45-51. doi: 10.11648/j.ijass.20130104.15 Abstract: In the present research work, we calculate the frequencies of Hawking radiations emitted from different test black holes existing in X-ray binaries (XRBs) and active galactic nuclei (AGN) by utilizing the proposed formula for the 8.037× 10 33 kg frequency of Hawking radiation f= Hz and show that these frequencies of Hawking radiations may be the M components of electromagnetic spectrum and gravitational waves. We also extend this work to convert the frequency of Hawking radiation in terms of the mass of the sun ( M ⊙ ) and then of Chandrasekhar limit ( M ch ), which is the largest unit of mass. Keywords: Electromagnetic Spectrum, Hawking Radiation, XRBs and AGN Starobinsky showed him that according to the quantum 1. -
Finding the Radiation from the Big Bang
Finding The Radiation from the Big Bang P. J. E. Peebles and R. B. Partridge January 9, 2007 4. Preface 6. Chapter 1. Introduction 13. Chapter 2. A guide to cosmology 14. The expanding universe 19. The thermal cosmic microwave background radiation 21. What is the universe made of? 26. Chapter 3. Origins of the Cosmology of 1960 27. Nucleosynthesis in a hot big bang 32. Nucleosynthesis in alternative cosmologies 36. Thermal radiation from a bouncing universe 37. Detecting the cosmic microwave background radiation 44. Cosmology in 1960 52. Chapter 4. Cosmology in the 1960s 53. David Hogg: Early Low-Noise and Related Studies at Bell Lab- oratories, Holmdel, N.J. 57. Nick Woolf: Conversations with Dicke 59. George Field: Cyanogen and the CMBR 62. Pat Thaddeus 63. Don Osterbrock: The Helium Content of the Universe 70. Igor Novikov: Cosmology in the Soviet Union in the 1960s 78. Andrei Doroshkevich: Cosmology in the Sixties 1 80. Rashid Sunyaev 81. Arno Penzias: Encountering Cosmology 95. Bob Wilson: Two Astronomical Discoveries 114. Bernard F. Burke: Radio astronomy from first contacts to the CMBR 122. Kenneth C. Turner: Spreading the Word — or How the News Went From Princeton to Holmdel 123. Jim Peebles: How I Learned Physical Cosmology 136. David T. Wilkinson: Measuring the Cosmic Microwave Back- ground Radiation 144. Peter Roll: Recollections of the Second Measurement of the CMBR at Princeton University in 1965 153. Bob Wagoner: An Initial Impact of the CMBR on Nucleosyn- thesis in Big and Little Bangs 157. Martin Rees: Advances in Cosmology and Relativistic Astro- physics 163. -
A Mathematical Appendix
381 A Mathematical Appendix A.1 Selected Formulae “Don’t worry about your difficulties in mathematics; I can assure you that mine are still greater.” Albert Einstein The solution of physics problems often involves mathemat- ics. In most cases nature is not so kind as to allow a precise mathematical treatment. Many times approximations are not only rather convenient but also necessary, because the gen- eral solution of specific problems can be very demanding and sometimes even impossible. In addition to these approximations, which often involve power series, where only the leading terms are relevant, ba- sic knowledge of calculus and statistics is required. In the following the most frequently used mathematical aids shall be briefly presented. 1. Power Series Binomial expansion: binomial expansion (1 ± x)m = m(m − 1) m(m − 1)(m − 2) 1 ± mx + x2 ± x3 +··· 2! 3! m(m − 1) ···(m − n + 1) + (±1)n xn +··· . n! For integer positive m this series is finite. The coefficients are binomial coefficients m(m − 1) ···(m − n + 1) m = . n! n If m is not a positive integer, the series is infinite and con- vergent for |x| < 1. This expansion often provides a simpli- fication of otherwise complicated expressions. 382 A Mathematical Appendix A few examples for most commonly used binomial ex- pansions: examples 1 1 1 5 (1 ± x)1/2 = 1 ± x − x2 ± x3 − x4 ±··· , for binomial expansions 2 8 16 128 − 1 3 5 35 (1 ± x) 1/2 = 1 ∓ x + x2 ∓ x3 + x4 ∓··· , 2 8 16 128 − (1 ± x) 1 = 1 ∓ x + x2 ∓ x3 + x4 ∓··· , (1 ± x)4 = 1 ± 4x + 6x2 ± 4x3 + x4 finite .