Where the Universe Came from How Einstein’S Relativity Unlocks the Past, Present and Future of the Cosmos
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FEATHERBEDDINGCOMPANYWEIN HOFJEREMIAHSTATUESYN AGOGEDREYFUSSMOOSCEMETERY MÜNSTERPLATZRELATIVI TYE=MC 2NOBELPRIZEHOMELAND PERSECUTIONAFFIDAVIT OFSUPPORTEMIGRATIONEINSTEIN STRASSELETTERSHOLOCAUSTRESCUE FAMILYGRANDMOTHERGRANDFAT HERBUCHAUPRINCETONBAHNHOF STRASSE20VOLKSHOCHSCHULEFOU NTAINGENIUSHUMANIST 01 Albert Einstein 6 7 Albert Einstein. More than just a name. Physicist. Genius. Science pop star. Philosopher and humanist. Thinker and guru. On a par with Copernicus, Galileo or Newton. And: Albert Einstein – from Ulm! The most famous scientist of our time was actually born on 14th March 1879 at Bahnhofstraße 20 in Ulm. Albert Einstein only lived in the city on the Danube for 15 months. His extended family – 18 of Einstein’s cousins lived in Ulm at one time or another – were a respected and deep-rooted part of the city’s society, however. This may explain Einstein’s enduring connection to the city of his birth, which he described as follows in a letter to the Ulmer Abend- post on 18th March 1929, shortly after his 50th birthday: “The birthplace is as much a unique part of your life as the ancestry of your biological mother. We owe part of our very being to our city of birth. So I look on Ulm with gratitude, as it combines noble artistic tradition with simple and healthy character.” 8 9 The “miracle year” 1905 – Einstein becomes the founder of the modern scientific world view Was Einstein a “physicist of the century”? There‘s no doubt of that. In his “miracle year” (annus mirabilis) of 1905 he pub- lished 4 groundbreaking works along- side his dissertation. Each of these was worthy of a Nobel Prize and turned him into a physicist of international standing: the theory of special relativity, the light quanta hypothesis (“photoelectric effect”), Thus, Albert Einstein became the found- for which he received the Nobel Prize in er of the modern scientific world view. -
A Study of Gravitational Wave Memory and Its Detectability with LIGO Using
A Study of Gravitational Wave Memory and Its Detectability With LIGO Using Bayesian Inference Interim Report #2 Jillian Doane - Oberlin College Mentors - Alan Weinstein and Jonah Kanner LIGO Document T1800230 LIGO SURF 2018 July 31, 2018 Update For Interim Report #2 I have made significant progress since my first interim report. I have accomplished the next steps I outlined in my previous interim report and I am also on track with the project schedule I made at the beginning of the year. So far I have met my expectations for the summer, and I am continuing to think about the next best step for my project. I have run into a few additional challenges since my last report. I have continued to have some issues with getting my code to work so I have had to take a substantial amount of time to debug. From this however I have built my intuition in regards to programming with Python which will be very beneficial for future projects and research. I have continued to use the same resources, mainly my mentors, tutorials, and the internet to answer questions and understand key concepts. The next step I am currently working on is creating a loop that will allow me to input a set of distance and mass parameters and plot them on the same graph. From here I will calculate the 90% confidence interval so I will be able to communicate how confident we are that lambda is equal to one. This calculation will also hopefully show that zero is not included at all in the peak which means that there is a very low probability that memory does not exist. -
SENTENARYO NG TEORYANG GENERAL RELATIVITY March 14, 2016 (1 - 3 Pm), NIP Auditorium, up Diliman Program Emcees: Ms
SENTENARYO NG TEORYANG GENERAL RELATIVITY March 14, 2016 (1 - 3 pm), NIP Auditorium, UP Diliman Program Emcees: Ms. Cherrie Olaya and Mr. Nestor Bareza National Anthem Welcome Remarks Academician William G. Padolina (NAST) Presentation 1 Einstein: Science, Image, and Impact (Dr. Perry Esguerra) Presentation 2 Einstein and the Music of the Spheres (Dr. Ian Vega) Intermission NIP Resonance Choir Presentation 3 From Einstein’s Universe to the Multiverse (Dr. Reina Reyes) Open Forum* *Moderators: Dr. May Lim and Dr. Nathaniel Hermosa II Closing Remarks Dr. Jose Maria P. Balmaceda (UP College of Science) (Refreshments will be served at the NIP Veranda) What’s Inside? Organizing Committee Messages p.1 Extended Abstracts 8 Dr. Percival Almoro (Chair) Einstein chronology 18 Dr. Perry Esguerra Einstein quotations 19 Dr. Ian Vega Dr. Caesar Saloma (Convenor) Outside Front Cover Outside Back Cover Inside Back Cover Einstein in Vienna, 1921 Depiction of gravitational waves Galaxies By: F. Schmutzer generated by binary neutron stars. By: Hubble Ultra Deep Field (Wikimedia Commons) By: R. Hurt/Caltech-JPL (http://hyperphysics.phy-astr.gsu. (http://www.jpl.nasa.gov/im- edu/hbase/astro/deepfield.html) ages/universe/20131106/pul- sar20131106-full.jpg) Acknowledgements Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 1 2 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 3 4 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) http://www.npr.org/sections/thetwo-way/2016/02/11/466286219/in-milestone- scientists-detect-waves-in-space-time-as-black-holes-collide https://www.youtube.com/watch?v=B4XzLDM3Py8 https://soundcloud.com/emily-lakdawalla Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 5 6 Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) Sentenaryo ng Teoryang General Relativity (March 14, 2016, UP-NIP) 7 Einstein: Science, Image, and Impact By Perry Esguerra ‘WHY is it that nobodY for photoluminescence, the ory of relativity. -
Albert Einstein - Wikipedia, the Free Encyclopedia Page 1 of 27
Albert Einstein - Wikipedia, the free encyclopedia Page 1 of 27 Albert Einstein From Wikipedia, the free encyclopedia Albert Einstein ( /ælbərt a nsta n/; Albert Einstein German: [albt a nʃta n] ( listen); 14 March 1879 – 18 April 1955) was a German-born theoretical physicist who developed the theory of general relativity, effecting a revolution in physics. For this achievement, Einstein is often regarded as the father of modern physics.[2] He received the 1921 Nobel Prize in Physics "for his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect". [3] The latter was pivotal in establishing quantum theory within physics. Near the beginning of his career, Einstein thought that Newtonian mechanics was no longer enough to reconcile the laws of classical mechanics with the laws of the electromagnetic field. This led to the development of his special theory of relativity. He Albert Einstein in 1921 realized, however, that the principle of relativity could also be extended to gravitational fields, and with his Born 14 March 1879 subsequent theory of gravitation in 1916, he published Ulm, Kingdom of Württemberg, a paper on the general theory of relativity. He German Empire continued to deal with problems of statistical Died mechanics and quantum theory, which led to his 18 April 1955 (aged 76) explanations of particle theory and the motion of Princeton, New Jersey, United States molecules. He also investigated the thermal properties Residence Germany, Italy, Switzerland, United of light which laid the foundation of the photon theory States of light. In 1917, Einstein applied the general theory of relativity to model the structure of the universe as a Ethnicity Jewish [4] whole. -
Einstein, Mileva Maric
ffirs.qrk 5/13/04 7:34 AM Page i Einstein A to Z Karen C. Fox Aries Keck John Wiley & Sons, Inc. ffirs.qrk 5/13/04 7:34 AM Page ii For Mykl and Noah Copyright © 2004 by Karen C. Fox and Aries Keck. All rights reserved Published by John Wiley & Sons, Inc., Hoboken, New Jersey Published simultaneously in Canada 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, scanning, or otherwise, except as permitted under Section 107 or 108 of the 1976 United States Copyright Act, without either the prior written permission of the Publisher, or authorization through payment of the appropriate per-copy fee to the Copyright Clearance Center, 222 Rosewood Drive, Danvers, MA 01923, (978) 750-8400, fax (978) 646-8600, or on the web at www.copyright.com. Requests to the Publisher for permission should be addressed to the Permissions Department, John Wiley & Sons, Inc., 111 River Street, Hoboken, NJ 07030, (201) 748-6011, fax (201) 748-6008. Limit of Liability/Disclaimer of Warranty: While the publisher and the author have used their best efforts in preparing this book, they make no representations or warranties with respect to the accuracy or completeness of the contents of this book and specifically disclaim any implied warranties of merchantability or fitness for a particular purpose. No warranty may be created or extended by sales representatives or written sales materials. The advice and strategies contained herein may not be suitable for your situation. -
Wave Detected by LIGO Is Not Gravitational Wave
Wave detected by LIGO is not gravitational wave Alfonso León Guillen Gómez Independent scientific researcher, Bogotá, Colombia E-mail: [email protected] Accepted by Journal of Modern Physics (JMP), 27 May 2016, Wulfenia Journal, 2 June 2016, and Jokull Journal, 8 September 2016, but not published, due to fee charges. Abstract General Relativity defines gravity like the metric of a Lorentzian manifold. Einstein formulated spacetime as quality structural of gravity, i.e, circular definition between gravity and spacetime, also Einstein denoted " Space and time are modes by which we think, not conditions under which we live " and “We denote everything but the gravitational field as matter”, therefore, spacetime is nothing and gravity in first approximation an effect of coordinates, and definitely a geometric effect. The mathematical model generates quantitative predictions coincident in high grade with observations without physical meaning. Philosophy intervened: in Substantivalism, spacetime exists in itself while in Relationalism as metrical relations. But, it does not know what spacetime. The outcomes of model have supported during a century, validity of the General Relativity, interpreted arbitrarily. Einstein formulated, from quadrupoles of energy, the formation of ripples in spacetime propagating as gravitational waves abandoned, in 1938, when he said that they do not exist. LIGO announced the first detection of gravitational waves from a pair of merging black holes. They truly are waves of quantum vacuum. KEYWORDS : Relativity, gravitational waves, quantum vacuum, mechanical quantum waves. PACS : 00-General 04. General relativity and gravitation 04.30.-w Gravitational waves 1 Introduction General Relativity keeps the two approaches of their authors since in its version called Entwurf was compound of the Physical Part of Albert Einstein and the Mathematical Part of Marcel Grossmann, being his equations limited generally covariant. -
Controversies in the History of the Radiation Reaction Problem in General Relativity
DIVISION OF THE HUMANITIES AND SOCIAL SCIENCES CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENA, CALIFORNIA 91125 CONTROVERSIES IN THE HISTORY OF THE RADIATION REACTION PROBLEM IN GENERAL RELATIVITY Daniel Kennefick ,.... 0 ...0 HUMANITIES WORKING PAPER 164 August 1996 Controversies in the History of the Radiation Reaction problem in General Relativity Daniel Kennefick* 1 Introduction Beginning in the early 1950s, experts in the theory of general relativity debated vigorously whether the theory predicted the emission of gravitational radiation from binary star systems. For a time, doubts also arose on whether gravitational waves could carry any energy. Since radiation phenomena have played a key role in the development of 20th century field theories, it is the main purpose of this paper to examine the reasons for the growth of scepticism regarding radiation in the case of the gravitational field. Although the focus is on the period from the mid-1930s to about 1960, when the modern study of gravitational waves was developing, some attention is also paid to the more recent and unexpected emergence of experimental data on gravitational waves which considerably sharpened the debate on certain controversial aspects of the theory of gravity waves. I analyze the use of the earlier history as a rhetorical device in review papers written by protagonists of the "quadrupole formula controversy" in the late 1970s and early 1980s. I argue that relativists displayed a lively interest in the historical background to the problem and exploited their knowledge of the literature to justify their own work and their assessment of the contemporary state of the subject. This illuminates the role of a scientific field's sense of its own history as a mediator in scientific controversy. -
Einstein's Dice and Schrödinger's
Free ebooks ==> www.Ebook777.com www.Ebook777.com Einstein’s Dice and Schrödinger’s Cat Free ebooks ==> www.Ebook777.com www.Ebook777.com Einstein’s Dice and Schrödinger’s Cat How Two Great Minds Battled Quantum Randomness to Create a Unifi ed Theory of Physics Paul Halpern, PhD A Member of the Perseus Books Group New York Free ebooks ==> www.Ebook777.com Copyright © 2015 by Paul Halpern Published by Basic Books, A Member of the Perseus Books Group All rights reserved. Printed in the United States of America. No part of this book may be reproduced in any manner whatsoever without written permission except in the case of brief quotations embodied in critical articles and reviews. For infor- mation, address Basic Books, 250 West 57th Street, New York, NY 10107. Books published by Basic Books are available at special discounts for bulk pur- chases in the United States by corporations, institutions, and other organizations. For more information, please contact the Special Markets Department at the Perseus Books Group, 2300 Chestnut Street, Suite 200, Philadelphia, PA 19103, or call (800) 810-4145, ext. 5000, or e-mail [email protected]. Designed by Pauline Brown Library of Congress Cataloging-in-Publication Data Halpern, Paul, 1961– Einstein’s dice and Schrödinger’s cat : how two great minds battled quantum randomness to create a unifi ed theory of physics / Paul Halpern, PhD. pages cm Includes bibliographical references and index. ISBN 978-0-465-07571-3 (hardcover) — ISBN 978-0-465-04065-0 (e-book) 1. Quantum chaos. 2. Quantum theory—Philosophy. 3. Physics—Philosophy. -
Einstein in Bern: the Great Legacy1
INTERNATIONAL SPACE SCIENCE INSTITUTE SPATIUM Published by the Association Pro ISSI No. 18, February 2007 SPATIUM 18 1 Editorial Omnia rerum principia parva sunt. Associate Professor at the Univer- The beginnings of all things are sity of Michigan have endeavoured Impressum small. successfully to translate the fascinat- ing ideas of Albert Einstein for a This famous quote of Marcus Tul- larger audience, not just in Bern, but lius Cicero is more than true for the in many stations all over the world middle drawer of an ordinary desk and to highlight some of the traces SPATIUM at the Kramgasse 49 in Bern. This he continues to leave in our daily Published by the drawer was called the office for the- life. We are greatly indebted to the Association Pro ISSI oretical physics by its owner, clearly authors for their kind permission to a euphemism initially, but more publish herewith a revised version than appropriate by the time when of their multi-media presentation. its contents prompted nothing less than a revolution of theoretical Association Pro ISSI physics. Hansjörg Schlaepfer Hallerstrasse 6, CH-3012 Bern Brissago, January 2007 Phone +41 (0)31 631 48 96 The desk belonged to the patent see clerk of third rank Albert Einstein, www.issibern.ch/pro-issi.html who during the office hours had to for the whole Spatium series treat the more or less ingenious in- ventions filed to the Patent Office, President while in his spare time had set out Prof. Heinrich Leutwyler to invent a new physics. University of Bern Layout and Publisher One might expect that such high- Dr. -
General Relativity
thinking about space and time: 100 years of applying and interpreting general relativity tuesday, sept 12 Wednesday, sept 13 thursday, sept 14 09.15-09.30 Welcome history ii cosmology ii and principles of gr cosmology i 09.15-10.00 Claus Kiefer (Köln) 09.15-10.30 Ruth Durrer (Geneva) Space and Time 62 years after the Bern Relativity Cosmology: The Problem of Dark Energy 09.30-10.45 Chris Smeenk (London, Ontario) Conference title tba 10.30-11.00 Coffee break 10.00-10.45 Sjang ten Hagen & Jeroen van Dongen (Amsterdam) 10.45-11.00 Coffee break Global Historiography and the Belgian Reception of 11.00-11.45 Ryan Samaroo (Bristol) 11.00-11.45 Cormac O’Raifeartaigh (Waterford) Relativity Friedman and Some of his Critics on the Foundations of Historical and Philosophical Aspects of the Einstein 10.45-11.15 Coffee break General Relativity World 11.45-12.30 Niels Linnemann (Geneva) 11.45-12.30 Casey D. McCoy (Edinburgh) 11.15-12.30 Marco Giovanelli (Tübingen) & Manus Visser (Amsterdam) A Thematic Tour of 20th Century Cosmology: Stability „All physics is Metaphysics“. On Émile Meyerson`s GR, quo vadis? - Indications for an Emergent Nature of From Einstein and Eddington to Infation Infuence on Einstein`s late Rationalistic Realism Gravity 12.30-14.00 Lunch break 12.30-14.00 Lunch break 12.30-14.00 Lunch break space-time and motion solutions to einstein’s field equations 14.00-14.45 Antonio Vassallo (Warsaw) Grounding as Metaphysical Causation in Spacetime 14.00-15.15 Jim Weatherall (Irvine) 14.00-15.15 Sabine Hossenfelder (Frankfurt) Physics Motion -
History of Gravitational Wave Emission
History of Gravitational Wave Emission Daniel Kennefick Univ. of Arkansas and Einstein Papers Project 6th Francis Bacon Conference, 2016 It has suddenly become a long history 1.3 billion years ago (very roughly) a binary system consisting of two roughly thirty solar mass black holes coalesced, sending out three solar masses of gravitational radiation. then now It has suddenly become a long history 1.3 billion years ago (very roughly) a binary system consisting of two roughly thirty solar mass black holes coalesced, sending out three solar masses of gravitational radiation. 21,040 years ago a binary neutron star system in our galaxy emitted gravitational waves which damped its own orbit enough for radio astronomers to detect the change using the Arecibo dish in Puerto Rico. then now It has suddenly become a long history 1.3 billion years ago (very roughly) a binary system consisting of two roughly thirty solar mass black holes coalesced, sending out three solar masses of gravitational radiation. 21,040 years ago a binary neutron star system in our galaxy emitted gravitational waves which damped its own orbit enough for radio astronomers to detect the change using the Arecibo antenna in Puerto Rico. 4,010 years ago another binary neutron star system (known as the double pulsar on Earth) exhibited very similar behavior which again convinces us the system is emitting gravitational waves in agreement with a formula worked out nearly a century ago by Albert Einstein then now A History of How we pieced this history together That history began 100 years and 22 days ago: “Since then, I have handled Newton's case differently, of course, according to the final theory. -
MITOCW | 17. Gravitational Radiation II
MITOCW | 17. Gravitational radiation II [SQUEAKING] [RUSTLING] [CLICKING] SCOTT OK. Let's move on to the next lecture. Might have gotten a little bit of me getting HUGHES: prepped here. I really have to give a lot of credit to the people in the Office of Digital Learning for making this entire thing possible. So I'm really grateful particularly to Elaine Mello, who is at home running the show remotely right now. This is-- a lot of people at MIT are doing a tremendous amount to keep this place functioning, and everyone really deserves a huge pat on the back. All right. So in the lecture that I just completed a few moments ago, we described-- I described how to characterize the gauge-invariant radiative degrees of freedom, which we call gravitational radiation. With gravitational radiation, we found at the end-- there's a formula that I will write down again a little bit later in this lecture, but we essentially found that it looks like certain projections of a term that involves two time derivatives of the quadrupole moment of a source. This has in recent years led to a-- well, we've now been able to directly measure this form of radiation. I'm wearing my LIGO hat in honor of the facility that first directly measured these things. And we have inaugurated an entirely new field of observational astronomy based on being able to measure those things. It's pretty exciting. I hope, though, that a few people noticed how restricted the analysis that I did is.