A View of Nature, Universe Where Are We Going?
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Vol 10 No 1, Winter 2004
SearchLites Vol. 10 No. 1, Winter 2004 The Quarterly Newsletter of The SETI League, Inc. Offices: 433 Liberty Street The Date Equation PO Box 555 by David Grinspoon Little Ferry NJ 07643 USA Editor's Note: This delightful analogy on the Drake Equation is excerpted from Dr. Grinspoon's new book Lonely Planets, ISBN 0-06-018540-6, © 2003, Harper Collins Publishers, New York. Phone: (201) 641-1770 Facsimile: Say you are a single person going to a large dance party, and you would like to come away with a (201) 641-1771 date for the following weekend. Arriving in front of the house, you can hear the music pumping Email: and feel the bass rattling your gut. You are excited, but nervous as hell, so you decide to calm [email protected] yourself with some math. Before going inside, you try to calculate your chances of getting lucky. Web: You start by guessing the total number of people at the party. You notice that people are arriving www.setileague.org at a rate of three per minute. We'll call this rate of arrival R. People are leaving at roughly the President: same rate, but you realize that you can estimate the number of people inside if you know how long Richard Factor they are staying. Let's call this length of stay L. The number of people inside will be roughly R Registered Agent: times L. So, if people on average are staying for, say, one hundred minutes, there will be about Marc Arnold, Esq. three hundred inside. -
PEN (Organization)
PEN (Organization): An Inventory of Its Records at the Harry Ransom Center Descriptive Summary Creator: PEN (Organization) Title: PEN (Organization) Records Dates: 1912-2008 (bulk 1926-1997) Extent: 352 document boxes, 5 card boxes (cb), 5 oversize boxes (osb) (153.29 linear feet), 4 oversize folders (osf) Abstract: The records of the London-based writers' organizations English PEN and PEN International, founded by Catharine Amy Dawson Scott in 1921, contain extensive correspondence with writer-members and other PEN centres around the world. Their records document campaigns, international congresses and other meetings, committees, finances, lectures and other programs, literary prizes awarded, membership, publications, and social events over several decades. Call Number: Manuscript Collection MS-03133 Language: The records are primarily written in English with sizeable amounts in French, German, and Spanish, and lesser amounts in numerous other languages. Non-English items are sometimes accompanied by translations. Note: The Ransom Center gratefully acknowledges the assistance of the National Endowment for the Humanities, which provided funds for the preservation, cataloging, and selective digitization of this collection. The PEN Digital Collection contains 3,500 images of newsletters, minutes, reports, scrapbooks, and ephemera selected from the PEN Records. An additional 900 images selected from the PEN Records and related Ransom Center collections now form five PEN Teaching Guides that highlight PEN's interactions with major political and historical trends across the twentieth century, exploring the organization's negotiation with questions surrounding free speech, political displacement, and human rights, and with global conflicts like World War II and the Cold War. Access: Open for research. Researchers must create an online Research Account and agree to the Materials Use Policy before using archival materials. -
Arxiv:1806.08561V1 [Cs.AI]
The Temporal Singularity: time-accelerated simulated civilizations and their implications Giacomo Spigler1 The Biorobotics Institute, Scuola Superiore Sant’Anna, Pisa, Italy, http://www.spigler.net/giacomo, [email protected] Abstract. Provided significant future progress in artificial intelligence and computing, it may ultimately be possible to create multiple Artificial General Intelligences (AGIs), and possibly entire societies living within simulated environments. In that case, it should be possible to improve the problem solving capabilities of the system by increasing the speed of the simulation. If a minimal simulation with sufficient capabilities is cre- ated, it might manage to increase its own speed by accelerating progress in science and technology, in a way similar to the Technological Singular- ity. This may ultimately lead to large simulated civilizations unfolding at extreme temporal speedups, achieving what from the outside would look like a Temporal Singularity. Here we discuss the feasibility of the mini- mal simulation and the potential advantages, dangers, and connection to the Fermi paradox of the Temporal Singularity. The medium-term im- portance of the topic derives from the amount of computational power required to start the process, which could be available within the next decades, making the Temporal Singularity theoretically possible before the end of the century. Keywords: temporal singularity; simulated civilization; multi-agent systems; simulated society; Fermi paradox; artificial life; technological singularity; arti- ficial general intelligence; deep reinforcement learning; simulation hypothesis; post-biological civilization 1 The Temporal Singularity arXiv:1806.08561v1 [cs.AI] 22 Jun 2018 It seems possible, if not likely, that artificial agents with general intelligence (AGI) will be built in the future [21,25]. -
1 the SUSTAINABILITY SOLUTION to the FERMI PARADOX Jacob D
THE SUSTAINABILITY SOLUTION TO THE FERMI PARADOX Jacob D. Haqq-Misra∗ Department of Meteorology & Astrobiology Research Center The Pennsylvania State University Seth D. Baum Department of Geography & Rock Ethics Institute The Pennsylvania State University No present observations suggest a technologically advanced extraterrestrial intelligence (ETI) has spread through the galaxy. However, under commonplace assumptions about galactic civilization formation and expansion, this absence of observation is highly unlikely. This improbability is the heart of the Fermi Paradox. The Fermi Paradox leads some to conclude that humans have the only advanced civilization in this galaxy, either because civilization formation is very rare or because intelligent civilizations inevitably destroy themselves. In this paper, we argue that this conclusion is premature by introducing the “Sustainability Solution” to the Fermi Paradox, which questions the Paradox’s assumption of faster (e.g. exponential) civilization growth. Drawing on insights from the sustainability of human civilization on Earth, we propose that faster-growth may not be sustainable on the galactic scale. If this is the case, then there may exist ETI that have not expanded throughout the galaxy or have done so but collapsed. These possibilities have implications for both searches for ETI and for human civilization management. ∗ Email address: [email protected] 1 1. INTRODUCTION The classic Fermi Paradox can lead to the conclusion that humans have formed the first advanced civilization in the galaxy because extraterrestrial intelligence (ETI) has not yet been observed [1]. Numerous resolutions to this paradox have been proposed [2], spanning the range of cosmological limits to sociological assumptions. A popular class of solutions assumes that the evolution of life is rare in the Universe: Earth may not be wholly unique, but other inhabited planets in the Universe could be too far away for any interaction or detection [3]. -
CUL Keller Archive Catalogue
HANS KELLER ARCHIVE: working copy A1: Unpublished manuscripts, 1940-49 A1/1: Unpublished manuscripts, 1940-49: independent work This section contains all Keller’s unpublished manuscripts dating from the 1940s, apart from those connected with his collaboration with Margaret Phillips (see A1/2 below). With the exception of one pocket diary from 1938, the Archive contains no material prior to his arrival in Britain at the end of that year. After his release from internment in 1941, Keller divided himself between musical and psychoanalytical studies. As a violinist, he gained the LRAM teacher’s diploma in April 1943, and was relatively active as an orchestral and chamber-music player. As a writer, however, his principal concern in the first half of the decade was not music, but psychoanalysis. Although the majority of the musical writings listed below are undated, those which are probably from this earlier period are all concerned with the psychology of music. Similarly, the short stories, poems and aphorisms show their author’s interest in psychology. Keller’s notes and reading-lists from this period indicate an exhaustive study of Freudian literature and, from his correspondence with Margaret Phillips, it appears that he did have thoughts of becoming a professional analyst. At he beginning of 1946, however, there was a decisive change in the focus of his work, when music began to replace psychology as his principal subject. It is possible that his first (accidental) hearing of Britten’s Peter Grimes played an important part in this change, and Britten’s music is the subject of several early articles. -
Fermi's Paradox-The Last Challenge for Copernicanism?
Fermi’s Paradox – The Last Challenge for Copernicanism? Milan M. Cirkovi´c´ Astronomical Observatory Belgrade, Volgina 7, 11160 Belgrade, Serbia & Department of Physics, University of Novi Sad, Trg Dositeja Obradovi´ca 4, 21000 Novi Sad, Serbia e-mail: [email protected] Abstract We review Fermi’s paradox (or the ”Great Silence” problem), not only arguably the oldest and crucial problem for the Search for ExtraTer- restrial Intelligence (SETI), but also a conundrum of profound scien- tific, philosophical and cultural importance. By a simple analysis of observation selection effects, the correct resolution of Fermi’s paradox is certain to tell us something about the future of humanity. Already a more than three quarters of a century old puzzle – and a quarter of century since the last major review paper in the field by G. David Brin – Fermi’s paradox has generated many ingenious discussions and hy- potheses. We analyze the often tacit methodological assumptions built into various answers to this puzzle and attempt a new classification of the numerous solutions proposed in an already huge literature on the subject. Finally, we consider the ramifications of various classes of hypotheses for the practical SETI projects. Somewhat paradoxically, it seems that the class of (neo)catastrophic hypotheses gives, on bal- ance, the strongest justification for guarded optimism regarding our current and near-future SETI efforts. Key words: astrobiology – extraterrestrial intelligence – Galaxy: evolution arXiv:0907.3432v1 [astro-ph.EP] 20 Jul 2009 – history and philosophy of astronomy – observation selection effects If you do not expect the unexpected, you will not find it; for it is hard to be sought out and difficult. -
Einstein for the 21St Century
Einstein for the 21st Century Einstein for the 21st Century HIS LEGACY IN SCIENCE, ART, AND MODERN CULTURE Peter L. Galison, Gerald Holton, and Silvan S. Schweber, Editors princeton university press | princeton and oxford Copyright © 2008 by Princeton University Press Published by Princeton University Press, 41 William Street, Princeton, New Jersey 08540 In the United Kingdom: Princeton University Press, 6 Oxford Street, Woodstock, Oxfordshire OX20 1TW All Rights Reserved Library of Congress Cataloging-in-Publication Data Einstein for the twenty-first century: His legacy in science, art, and modern culture / Peter L. Galison, Gerald Holton, and Silvan S. Schweber, editors. p. cm. Includes bibliographical references and index. ISBN 978-0-691-13520-5 (hardcover : acid-free paper) 1. Einstein, Albert, 1879–1955—Influence. I. Galison, Peter Louis. II. Holton, Gerald James. III. Schweber, S. S. (Silvan S.) IV. Title: Einstein for the 21st century. QC16.E5E446 2008 530.092—dc22 2007034853 British Library Cataloging-in-Publication Data is available This book has been composed in Aldus and Trajan Printed on acid-free paper. ∞ press.princeton.edu Printed in the United States of America 13579108642 Contents Introduction ix part 1 Solitude and World 1 Who Was Einstein? Why Is He Still So Alive? 3 Gerald Holton 2 A Short History of Einstein’s Paradise beyond the Personal 15 Lorraine Daston 3 Einstein’s Jewish Identity 27 Hanoch Gutfreund 4 Einstein and God 35 Yehuda Elkana 5 Einstein’s Unintended Legacy: The Critique of Common-Sense Realism and Post-Modern Politics 48 Yaron Ezrahi 6 Subversive Einstein 59 Susan Neiman 7 Einstein and Nuclear Weapons 72 Silvan S. -
Wij-Articles-Corrected Russian Dolls-1
Russian Dolls RUSSIAN DOLLS: THE POLIANOWSKI SISTERS’ MEMOIRS ON ALBERT EINSTEIN AND LUDWIG WITTGENSTEIN Ann Lazarsfeld-Jensen, Charles Sturt University, Bathurst NSW, Australia ABSTRACT In the 1970’s two Russian sisters wrote their memoirs of working with Albert Einstein and Ludwig Wittgenstein in long essays published in the trans Atlantic literary journal, Encounter. The intimacy of their experience with both men conflicts with the public image of misogynists given to callous expressions of their prejudice. The Polianowski sisters, Esther and Fania, had suffered the indignities of being born female at the fin de siecle despite the progressive attitude to the education of women in the Ukraine. They were cynical but tolerant of sexual discrimination perhaps because their lives had been torn apart by the greater terror of anti-Semitism that had driven them across Europe. It was their Jewish identity and suffering that inspired some significant intellectuals to befriend them including Dr. Redcliffe Salaman, Frances Cornford and Shlomo Bardin, and brought them into the circle of the scholars they married. That they had independently escaped and survived inspired awe even in a man like Einstein. The Polianowski women were included in academic circles at Cambridge University between the wars, and they found meaningful work teaching Russian, and married professors Myer Salaman and Roy Pascal. Using a comparative historical approach to the life and writing of Esther Salaman and Fania Pascal, this article demonstrates that Jewish identity moderated gender bias among significant intellectuals in the 20th century giving marginalised women a measure of opportunity. However, it was limited opportunity. The Polianowski women did not achieve the careers they respectively planned in physics and philosophy, and their contribution as writers is not well recognised. -
Aliens!!! We Have One Data Point: No One Has Ever Detected an Alien
Aliens!!! We have one data point: no one has ever detected an alien: 1. No personal contact 2. No detection of alien ships/artifacts on Earth or elsewhere 3. No detection of signals of extraterrestrial origin Can we ask any scientific questions about aliens? A gray area between science and science fiction 1. Can we estimate the likelihood of alien life? 2. How might extraterrestrial life adapt to extreme environments? Estimating the abundance of alien life: A “back of the envelope calculation” or a “Fermi Problem” How much coal would it take to power the US for a year? How many air travellers are in the air right now? How many piano tuners are there in Chicago? The original Fermi Problem: How many piano tuners live in Chicago? How many people live in Chicago? 9 million How many households in Chicago? 4.5 million (2 people per household) How many households have pianos that get tuned regularly? (1 out of 20) = 225,000 tunings per year A typical work year is 2000 hours, and it takes about 2 hours to tune a piano, so a piano tuner does 1000 tunings in a year. So Chicago employs about 200 piano tuners How many aliens are there?? 1. How many stars are in the galaxy? 2. How many of these stars have planets? 3. How many planets develop life? 4. How many planets with life develop intelligent life? 5. How many of the intelligent aliens will broadcast their existence? The (in)famous Drake Equation: N = R* · fp · ne · fl · fi · fc · L If intelligent life is common, where are all the aliens? The “Fermi paradox” Solutions to the Fermi Paradox: 1. -
Where Is Everybody? If the Universe Is Teeming with Aliens
IF THE UNIVERSE IS TEEMING WITH ALIENS ... WHERE IS EVERYBODY? IF THE UNIVERSE IS TEEMING WITH ALIENS ... WHERE IS EVERYBODY? FIFTY SOLUTIONS TO THE FERMI PARADOX AND THE PROBLEM OF EXTRATERRESTRIAL LIFE Stephen Webb Copernicus Books IN ASSOCIATION WITH Praxis Publishing Ltd. An Imprint of Springer-Verlag © Praxis Publishing Ltd, 2002. All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording, or other- wise, without the prior written permission of the publisher. Published in the United States by Copernicus Books, an imprint of Springer-Verlag New York, Inc. A member of BertelsmannSpringer Science+Business Media GmbH Copernicus Books 37 East 7th Street New York, NY 10003 www.copernicusbooks.com Library of Congress Cataloging-in-Publication Data Webb, Stephen. If the universe is teeming with aliens . where is everybody? : fifty solutions to the Fermi paradox and the problem of extraterrestrial life / Stephen Webb. p. cm. Includes bibliographical references and index. ISBN 0-387-95501-1 (acid-free paper) 1. Fermi paradox. 2. Life on other planets. 3. Fermi, Enrico, 1901–1945. I. Title. QB54.W384 2002 576.8’39—dc21 2002073910 Manufactured in the United States of America. Printed on acid-free paper. 987654321 ISBN 0-387-95501-1 SPIN 10879967 To Heike CONTENTS Preface ix Figure Credits xi Chapter 1 Where Is Everybody? 1 Chapter 2 Of Fermi and Paradox 7 Enrico Fermi 8 Paradox 12 The Fermi Paradox 17 Chapter 3 They -
DISCOVERY and VALIDATION of Kepler-452B: a 1.6-R⊕ SUPER EARTH EXOPLANET in the HABITABLE ZONE of a G2 STAR Jon M
Received 2015 March 3; accepted 2015 May 23; published 2015 July 23 by the Astronomical Journal Preprint typeset using LATEX style emulateapj v. 12/16/11 DISCOVERY AND VALIDATION OF Kepler-452b: A 1:6-R⊕ SUPER EARTH EXOPLANET IN THE HABITABLE ZONE OF A G2 STAR Jon M. Jenkins1, Joseph D. Twicken1,2, Natalie M. Batalha1, Douglas A. Caldwell1,2, William D. Cochran3, Michael Endl3, David W. Latham4, Gilbert A. Esquerdo4, Shawn Seader1,2, Allyson Bieryla4, Erik Petigura5, David R. Ciardi6, Geoffrey W. Marcy5, Howard Isaacson5, Daniel Huber7,2,8, Jason F. Rowe1,2, Guillermo Torres4, Stephen T. Bryson1, Lars Buchhave4,9, Ivan Ramirez3, Angie Wolfgang10, Jie Li1,2, Jennifer R. Campbell11, Peter Tenenbaum1,2, Dwight Sanderfer1 Christopher E. Henze1, Joseph H. Catanzarite1,2, Ronald L. Gilliland12, and William J. Borucki1 Received 2015 March 3; accepted 2015 May 23; published 2015 July 23 by the Astronomical Journal ABSTRACT We report on the discovery and validation of Kepler-452b, a transiting planet identified by a search +0:23 through the 4 years of data collected by NASA's Kepler Mission. This possibly rocky 1:63−0:20-R⊕ +0:007 planet orbits its G2 host star every 384:843−0:012 days, the longest orbital period for a small (RP < 2 R⊕) transiting exoplanet to date. The likelihood that this planet has a rocky composition lies between 49% and 62%. The star has an effective temperature of 5757 ± 85 K and a log g of 4:32 ± 0:09. At +0:019 a mean orbital separation of 1:046−0:015 AU, this small planet is well within the optimistic habitable zone of its star (recent Venus/early Mars), experiencing only 10% more flux than Earth receives from the Sun today, and slightly outside the conservative habitable zone (runaway greenhouse/maximum +0:15 greenhouse). -
Fermi Paradox from Wikipedia, the Free Encyclopedia Jump To: Navigation, Search
Fermi paradox From Wikipedia, the free encyclopedia Jump to: navigation, search This article is about the absence of evidence for extraterrestrial intelligence. For the type of estimation problem, see Fermi problem. For the music album, see Fermi Paradox (album). For the short story, see The Fermi Paradox Is Our Business Model. A graphical representation of the Arecibo message – Humanity's first attempt to use radio waves to actively communicate its existence to alien civilizations The Fermi paradox (or Fermi's paradox) is the apparent contradiction between high estimates of the probability of the existence of extraterrestrial civilization and humanity's lack of contact with, or evidence for, such civilizations.[1] The basic points of the argument, made by physicists Enrico Fermi and Michael H. Hart, are: • The Sun is a young star. There are billions of stars in the galaxy that are billions of years older; • Some of these stars likely have Earth-like planets[2] which, if the Earth is typical, may develop intelligent life; • Presumably some of these civilizations will develop interstellar travel, as Earth seems likely to do; • At any practical pace of interstellar travel, the galaxy can be completely colonized in just a few tens of millions of years. According to this line of thinking, the Earth should have already been colonized, or at least visited. But no convincing evidence of this exists. Furthermore, no confirmed signs of intelligence elsewhere have been spotted, either in our galaxy or the more than 80 billion other galaxies of the