If the Universe Is Teeming with Aliens… WHERE IS EVERYBODY?
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Modelling Panspermia in the TRAPPIST-1 System
October 13, 2017 Modelling panspermia in the TRAPPIST-1 system James A. Blake1,2*, David J. Armstrong1,2, Dimitri Veras1,2 Abstract The recent ground-breaking discovery of seven temperate planets within the TRAPPIST-1 system has been hailed as a milestone in the development of exoplanetary science. Centred on an ultra-cool dwarf star, the planets all orbit within a sixth of the distance from Mercury to the Sun. This remarkably compact nature makes the system an ideal testbed for the modelling of rapid lithopanspermia, the idea that micro-organisms can be distributed throughout the Universe via fragments of rock ejected during a meteoric impact event. We perform N-body simulations to investigate the timescale and success-rate of lithopanspermia within TRAPPIST-1. In each simulation, test particles are ejected from one of the three planets thought to lie within the so-called ‘habitable zone’ of the star into a range of allowed orbits, constrained by the ejection velocity and coplanarity of the case in question. The irradiance received by the test particles is tracked throughout the simulation, allowing the overall radiant exposure to be calculated for each one at the close of its journey. A simultaneous in-depth review of space microbiological literature has enabled inferences to be made regarding the potential survivability of lithopanspermia in compact exoplanetary systems. 1Department of Physics, University of Warwick, Coventry, CV4 7AL 2Centre for Exoplanets and Habitability, University of Warwick, Coventry, CV4 7AL *Corresponding author: [email protected] Contents Universe, and can propagate from one location to another. This interpretation owes itself predominantly to the works of William 1 Introduction1 Thompson (Lord Kelvin) and Hermann von Helmholtz in the 1.1 Mechanisms for panspermia...............2 latter half of the 19th Century. -
Mathematical Anthropology and Cultural Theory
UCLA Mathematical Anthropology and Cultural Theory Title SOCIALITY IN E. O. WILSON’S GENESIS: EXPANDING THE PAST, IMAGINING THE FUTURE Permalink https://escholarship.org/uc/item/7p343150 Journal Mathematical Anthropology and Cultural Theory, 14(1) ISSN 1544-5879 Author Denham, Woodrow W Publication Date 2019-10-01 Peer reviewed eScholarship.org Powered by the California Digital Library University of California MATHEMATICAL ANTHROPOLOGY AND CULTURAL THEORY: AN INTERNATIONAL JOURNAL VOLUME 14 NO. 1 OCTOBER 2019 SOCIALITY IN E. O. WILSON’S GENESIS: EXPANDING THE PAST, IMAGINING THE FUTURE. WOODROW W. DENHAM, Ph. D. RETIRED INDEPENDENT SCHOLAR [email protected] COPYRIGHT 2019 ALL RIGHTS RESERVED BY AUTHOR SUBMITTED: AUGUST 16, 2019 ACCEPTED: OCTOBER 1, 2019 MATHEMATICAL ANTHROPOLOGY AND CULTURAL THEORY: AN INTERNATIONAL JOURNAL ISSN 1544-5879 DENHAM: SOCIALITY IN E. O. WILSON’S GENESIS WWW.MATHEMATICALANTHROPOLOGY.ORG MATHEMATICAL ANTHROPOLOGY AND CULTURAL THEORY: AN INTERNATIONAL JOURNAL VOLUME 14, NO. 1 PAGE 1 OF 37 OCTOBER 2019 Sociality in E. O. Wilson’s Genesis: Expanding the Past, Imagining the Future. Woodrow W. Denham, Ph. D. Abstract. In this article, I critique Edward O. Wilson’s (2019) Genesis: The Deep Origin of Societies from a perspective provided by David Christian’s (2016) Big History. Genesis is a slender, narrowly focused recapitulation and summation of Wilson’s lifelong research on altruism, eusociality, the biological bases of kinship, and related aspects of sociality among insects and humans. Wilson considers it to be among the most important of his 35+ published books, one of which created the controversial discipline of sociobiology and two of which won Pulitzer Prizes. -
The Cosmos - Before the Big Bang
From issue 2601 of New Scientist magazine, 28 April 2007, page 28-33 The cosmos - before the big bang How did the universe begin? The question is as old as humanity. Sure, we know that something like the big bang happened, but the theory doesn't explain some of the most important bits: why it happened, what the conditions were at the time, and other imponderables. Many cosmologists think our standard picture of how the universe came to be is woefully incomplete or even plain wrong, and they have been dreaming up a host of strange alternatives to explain how we got here. For the first time, they are trying to pin down the initial conditions of the big bang. In particular, they want to solve the long-standing mystery of how the universe could have begun in such a well- ordered state, as fundamental physics implies, when it seems utter chaos should have reigned. Several models have emerged that propose intriguing answers to this question. One says the universe began as a dense sea of black holes. Another says the big bang was sparked by a collision between two membranes floating in higher-dimensional space. Yet another says our universe was originally ripped from a larger entity, and that in turn countless baby universes will be born from the wreckage of ours. Crucially, each scenario makes unique and testable predictions; observations coming online in the next few years should help us to decide which, if any, is correct. Not that modelling the origin of the universe is anything new. -
Technical Proposal for Onsite Destruction of Stored Waste on Vertac Site
ichnicol Proposal to Arkansas Department of dilution Control and Ecology )rthe )N-SITE DESTRUCTION OF STORED VASTE ON TNE VERTAC SITE IN ACKSONVILLE, ARKANSAS ugust13,1987 ^ WESTINGHOUSE ELECTRIC CORPORATION Environmental Technology Division iZTECH INC. Westinghouse Power Systems Box 286 Electric Corporation Business Unit Madison Pennsylvania 15663-0286 E P Rahe Jr General Manager Environmental Technology Division •August 13. 1987 ^ \ A ^ Mr. Paul Mean Director Arkansas Department of Pollution Control and Ecology 8001 National Drive P.O. Box 9583 Little Rock, AR 72209 Subject: Technical Proposal for Destruction of Stored Waste on the Vertac Site in Jacksonville, Arkansas Dear Mr. Mean: Vestinghouse Electric Corporation and HAZTECH, Inc. are pleased to submit the attached technical proposal for the on-site destruction of the stored waste on the Vertac site in Jacksonville, Arkansas. The proposal addresses three options for the handling and destruction of all materials stored above ground on the site. Vestinghouse will be the project manager for all work on site. The recommended option is to destroy the liquid or crystalline material using the Vestinghouse Pyroplasma process which is a thermal treatment technology. The system uses a plasma torch which produces Cemperatures between 5000°C and 15,000°C. The most important advantages of this process, relative to combustion processes, are very low emissions, very high destruction efficiencies, and low PIC (product of incomplete combustion) formation. In addition, this system is truly mobile. All of the process equipment is contained in one 48-foot trailer and can be sec up on site within one week. Ve believe that the Pyroplasaa destruction process is very well suited for your specific waste material. -
Quantum Cosmology of the Big Rip: Within GR and in a Modified Theory of Gravity
universe Conference Report Quantum Cosmology of the Big Rip: Within GR and in a Modified Theory of Gravity Mariam Bouhmadi-López 1,2,*, Imanol Albarran 3,4 and Che-Yu Chen 5,6 1 Department of Theoretical Physics, University of the Basque Country UPV/EHU, P.O. Box 644, 48080 Bilbao, Spain 2 IKERBASQUE, Basque Foundation for Science, 48011 Bilbao, Spain 3 Departamento de Física, Universidade da Beira Interior, Rua Marquês D’Ávila e Bolama, 6201-001 Covilhã, Portugal; [email protected] 4 Centro de Matemática e Aplicações da Universidade da Beira Interior (CMA-UBI), Rua Marquês D’Ávila e Bolama, 6201-001 Covilhã, Portugal 5 Department of Physics, National Taiwan University, 10617 Taipei, Taiwan; [email protected] 6 LeCosPA, National Taiwan University, 10617 Taipei, Taiwan * Correspondence: [email protected] Academic Editors: Mariusz P. D ˛abrowski, Manuel Krämer and Vincenzo Salzano Received: 8 March 2017; Accepted: 12 April 2017; Published: 14 April 2017 Abstract: Quantum gravity is the theory that is expected to successfully describe systems that are under strong gravitational effects while at the same time being of an extreme quantum nature. When this principle is applied to the universe as a whole, we use what is commonly named “quantum cosmology”. So far we do not have a definite quantum theory of gravity or cosmology, but we have several promising approaches. Here we will review the application of the Wheeler–DeWitt formalism to the late-time universe, where it might face a Big Rip future singularity. The Big Rip singularity is the most virulent future dark energy singularity which can happen not only in general relativity but also in some modified theories of gravity. -
Exotic Beasts
Searching for Extraterrestrial Intelligence Beyond the Milky Way The first Swedish SETI project Erik Zackrisson Department of Astronomy Oskar Klein Centre Searching for Extraterrestrial Intelligence (SETI) – A Brief History I • 1959 – Cocconi & Morrison (Nature): ”Try the hydrogen frequency (1.42 GHz)” • 1960 – Project Ozma • 1961 – Schwartz & Townes (Nature): ”Try optical laser” • 1977 – The Wow signal Searching for Extraterrestrial Intelligence (SETI) – A Brief History II • 1984 – The SETI Institute • Late 1990s – Optical SETI becomes popular • 1999 – SETI@home • 2007 – Allen Telescope Array • 2012 – SETI Live The Fermi Paradox • No signals from E.T. despite 50 years of SETI • The Milky Way can be colonized in 1% of its current age – why are we not already colonized? • Where is everybody? 50+ possible solutions are known (e.g. Brin 1983, Webb 2002) A Few Possible Explanations • Everybody is staying at home and nobody is transmitting – Virtual worlds more exciting than space exploration? – Berserkers Transmission = Doom • Wrong search strategy – Try artefacts, Bracewell probes, IR laser, internet, DNA, Dyson spheres… • Intelligent life is extremely rare – Try extragalactic SETI Beyond the Milky Way • Carl Sagan: ”More stars in the Universe than grains of sand on all the beaches on Earth” • Stars in Milky Way 1011 • Stars in observable Universe 1023 Only a handful of extragalactic SETI projects carried out so far! Earth-like planets in a cosmological context I Millenium simulation + Semi-analytic galaxy models + Metallicity-dependent -
Interstellar Communication: the Case for Spread Spectrum
Interstellar Communication: The Case for Spread Spectrum David G Messerschmitta aDepartment of Electrical Engineering and Computer Sciences, 253 Cory Hall, University of California, Berkeley, California 94720-1770, USA, [email protected], 1-925-465-5740 Abstract Spread spectrum, widely employed in modern digital wireless terrestrial radio systems, chooses a signal with a noise-like character and much higher bandwidth than necessary. This paper advocates spread spectrum modulation for interstellar communication, motivated by robust immunity to radio- frequency interference (RFI) of technological origin in the vicinity of the receiver while preserving full detection sensitivity in the presence of natural sources of noise. Receiver design for noise immunity alone provides no basis for choosing a signal with any specific character, therefore failing to reduce ambiguity. By adding RFI to noise immunity as a design objective, the conjunction of choice of signal (by the transmitter) together with optimum detection for noise immunity (in the receiver) leads through simple probabilistic argument to the conclusion that the signal should possess the statistical properties of a burst of white noise, and also have a large time-bandwidth product. Thus spread spectrum also provides an implicit coordination between transmitter and receiver by reducing the ambiguity as to the signal character. This strategy requires the receiver to guess the specific noise-like signal, and it is contended that this is feasible if an appropriate pseudorandom signal is generated algorithmically. For example, conceptually simple algorithms like the binary expansion of common irrational numbers like π are shown to be suitable. Due to its deliberately wider bandwidth, spread spectrum is more susceptible to dispersion and distortion in propagation through the interstellar medium, desirably reducing ambiguity in parameters like bandwidth and carrier frequency. -
The Search for Extraterrestrial Intelligence
THE SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE Are we alone in the universe? Is the search for extraterrestrial intelligence a waste of resources or a genuine contribution to scientific research? And how should we communicate with other life-forms if we make contact? The search for extraterrestrial intelligence (SETI) has been given fresh impetus in recent years following developments in space science which go beyond speculation. The evidence that many stars are accompanied by planets; the detection of organic material in the circumstellar disks of which planets are created; and claims regarding microfossils on Martian meteorites have all led to many new empirical searches. Against the background of these dramatic new developments in science, The Search for Extraterrestrial Intelligence: a philosophical inquiry critically evaluates claims concerning the status of SETI as a genuine scientific research programme and examines the attempts to establish contact with other intelligent life-forms of the past thirty years. David Lamb also assesses competing theories on the origin of life on Earth, discoveries of ex-solar planets and proposals for space colonies as well as the technical and ethical issues bound up with them. Most importantly, he considers the benefits and drawbacks of communication with new life-forms: how we should communicate and whether we could. The Search for Extraterrestrial Intelligence is an important contribution to a field which until now has not been critically examined by philosophers. David Lamb argues that current searches should continue and that space exploration and SETI are essential aspects of the transformative nature of science. David Lamb is honorary Reader in Philosophy and Bioethics at the University of Birmingham. -
Exploring Biogenic Dispersion Inside Star Clusters with System Dynamics Modeling
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 12 October 2020 doi:10.20944/preprints202010.0232.v1 Exploring Biogenic Dispersion Inside Star Clusters with System Dynamics Modeling Authors Javier D. Burgos. Corporación para la Investigacion e Innovación -CIINAS. Contact: [email protected] Diana C. Sierra. Corporación para la Investigacion e Innovación -CIINAS; Bogotá, Colombia. Contact: [email protected] Abstract The discovery of a growing number of exoplanets and even extrasolar systems supports the scientific consensus that it is possible to find other signs of life in the universe. The present work proposes for the first time, an explicit mechanism inspired by the dynamics of biological dispersion, widely used in ecology and epidemiology, to study the dispersion of biogenic units, interpreted as complex organic molecules, between rocky or water exoplanets (habitats) located inside star clusters. The 3 results of the dynamic simulation suggest that for clusters with populations lower than 4 M/ly it is not possible to obtain biogenic worlds after 5 Gyr. Above this population size, biogenic dispersion seems to follow a power law, the larger the density of worlds lesser will be the impact rate (훽.) value to obtain at least one viable biogenic Carrier habitat after 5 Gyr. Finally, when we investigate scenarios by varying β, a well-defined set of density intervals can be defined in accordance to its characteristic β value, suggesting that biogenic dispersion has a behavior of “minimal infective dose” of “minimal biogenic effective” events by interval i.e. once this dose has been achieved, doesn’t matter if additional biogenic impact events occur on the habitat. -
God and Design: the Teleological Argument and Modern Science
GOD AND DESIGN Is there reason to think a supernatural designer made our world? Recent discoveries in physics, cosmology, and biochemistry have captured the public imagination and made the design argument—the theory that God created the world according to a specific plan—the object of renewed scientific and philosophical interest. Terms such as “cosmic fine-tuning,” the “anthropic principle,” and “irreducible complexity” have seeped into public consciousness, increasingly appearing within discussion about the existence and nature of God. This accessible and serious introduction to the design problem brings together both sympathetic and critical new perspectives from prominent scientists and philosophers including Paul Davies, Richard Swinburne, Sir Martin Rees, Michael Behe, Elliott Sober, and Peter van Inwagen. Questions raised include: • What is the logical structure of the design argument? • How can intelligent design be detected in the Universe? • What evidence is there for the claim that the Universe is divinely fine-tuned for life? • Does the possible existence of other universes refute the design argument? • Is evolutionary theory compatible with the belief that God designed the world? God and Design probes the relationship between modern science and religious belief, considering their points of conflict and their many points of similarity. Is God the “master clockmaker” who sets the world’s mechanism on a perfectly enduring course, or a miraculous presence continually intervening in and altering the world we know? Are science and faith, or evolution and creation, really in conflict at all? Expanding the parameters of a lively and urgent contemporary debate, God and Design considers the ways in which perennial questions of origin continue to fascinate and disturb us. -
Monday, November 13, 2017 WHAT DOES IT MEAN to BE HABITABLE? 8:15 A.M. MHRGC Salons ABCD 8:15 A.M. Jang-Condell H. * Welcome C
Monday, November 13, 2017 WHAT DOES IT MEAN TO BE HABITABLE? 8:15 a.m. MHRGC Salons ABCD 8:15 a.m. Jang-Condell H. * Welcome Chair: Stephen Kane 8:30 a.m. Forget F. * Turbet M. Selsis F. Leconte J. Definition and Characterization of the Habitable Zone [#4057] We review the concept of habitable zone (HZ), why it is useful, and how to characterize it. The HZ could be nicknamed the “Hunting Zone” because its primary objective is now to help astronomers plan observations. This has interesting consequences. 9:00 a.m. Rushby A. J. Johnson M. Mills B. J. W. Watson A. J. Claire M. W. Long Term Planetary Habitability and the Carbonate-Silicate Cycle [#4026] We develop a coupled carbonate-silicate and stellar evolution model to investigate the effect of planet size on the operation of the long-term carbon cycle, and determine that larger planets are generally warmer for a given incident flux. 9:20 a.m. Dong C. F. * Huang Z. G. Jin M. Lingam M. Ma Y. J. Toth G. van der Holst B. Airapetian V. Cohen O. Gombosi T. Are “Habitable” Exoplanets Really Habitable? A Perspective from Atmospheric Loss [#4021] We will discuss the impact of exoplanetary space weather on the climate and habitability, which offers fresh insights concerning the habitability of exoplanets, especially those orbiting M-dwarfs, such as Proxima b and the TRAPPIST-1 system. 9:40 a.m. Fisher T. M. * Walker S. I. Desch S. J. Hartnett H. E. Glaser S. Limitations of Primary Productivity on “Aqua Planets:” Implications for Detectability [#4109] While ocean-covered planets have been considered a strong candidate for the search for life, the lack of surface weathering may lead to phosphorus scarcity and low primary productivity, making aqua planet biospheres difficult to detect. -
Closed Timelike Curves, Singularities and Causality: a Survey from Gödel to Chronological Protection
Closed Timelike Curves, Singularities and Causality: A Survey from Gödel to Chronological Protection Jean-Pierre Luminet Aix-Marseille Université, CNRS, Laboratoire d’Astrophysique de Marseille , France; Centre de Physique Théorique de Marseille (France) Observatoire de Paris, LUTH (France) [email protected] Abstract: I give a historical survey of the discussions about the existence of closed timelike curves in general relativistic models of the universe, opening the physical possibility of time travel in the past, as first recognized by K. Gödel in his rotating universe model of 1949. I emphasize that journeying into the past is intimately linked to spacetime models devoid of timelike singularities. Since such singularities arise as an inevitable consequence of the equations of general relativity given physically reasonable assumptions, time travel in the past becomes possible only when one or another of these assumptions is violated. It is the case with wormhole-type solutions. S. Hawking and other authors have tried to save the paradoxical consequences of time travel in the past by advocating physical mechanisms of chronological protection; however, such mechanisms remain presently unknown, even when quantum fluctuations near horizons are taken into account. I close the survey by a brief and pedestrian discussion of Causal Dynamical Triangulations, an approach to quantum gravity in which causality plays a seminal role. Keywords: time travel; closed timelike curves; singularities; wormholes; Gödel’s universe; chronological protection; causal dynamical triangulations 1. Introduction In 1949, the mathematician and logician Kurt Gödel, who had previously demonstrated the incompleteness theorems that broke ground in logic, mathematics, and philosophy, became interested in the theory of general relativity of Albert Einstein, of which he became a close colleague at the Institute for Advanced Study at Princeton.