A Brief History of Gravitational Waves

Total Page:16

File Type:pdf, Size:1020Kb

A Brief History of Gravitational Waves Review A Brief History of Gravitational Waves Jorge L. Cervantes-Cota 1, Salvador Galindo-Uribarri 1 and George F. Smoot 2,3,4,* 1 Department of Physics, National Institute for Nuclear Research, Km 36.5 Carretera Mexico-Toluca, Ocoyoacac, Mexico State C.P.52750, Mexico; [email protected] (J.L.C.-C.); [email protected] (S.G.-U.) 2 Helmut and Ana Pao Sohmen Professor at Large, Institute for Advanced Study, Hong Kong University of Science and Technology, Clear Water Bay, 999077 Kowloon, Hong Kong, China. 3 Université Sorbonne Paris Cité, Laboratoire APC-PCCP, Université Paris Diderot, 10 rue Alice Domon et Leonie Duquet 75205 Paris Cedex 13, France. 4 Department of Physics and LBNL, University of California; MS Bldg 50-5505 LBNL, 1 Cyclotron Road Berkeley, CA 94720, USA. * Correspondence: [email protected]; Tel.:+1-510-486-5505 Abstract: This review describes the discovery of gravitational waves. We recount the journey of predicting and finding those waves, since its beginning in the early twentieth century, their prediction by Einstein in 1916, theoretical and experimental blunders, efforts towards their detection, and finally the subsequent successful discovery. Keywords: gravitational waves; General Relativity; LIGO; Einstein; strong-field gravity; binary black holes 1. Introduction Einstein’s General Theory of Relativity, published in November 1915, led to the prediction of the existence of gravitational waves that would be so faint and their interaction with matter so weak that Einstein himself wondered if they could ever be discovered. Even if they were detectable, Einstein also wondered if they would ever be useful enough for use in science. However, exactly 100 years after his theory was born, on 14 September 2015, these waves were finally detected and are going to provide scientific results. In fact at 11:50:45 am CET on 14 September 2015 Marco Drago—a postdoc —was seated in front of a computer monitor at the Max Planck Institute for Gravitational Physics in Hanover, Germany, when he received an e-mail, automatically generated three minutes before from the monitors of LIGO (for its acronym Laser Interferometer Gravitational wave Observatory). Marco opened the e-mail, which contained two links. He opened both links and each contained a graph of a signal similar to that recorded by ornithologists to register the songs of birds. One graph came from a LIGO station located at Hanford, in Washington State, and the other from Livingston Station in the state of Louisiana [1]. (a) (b) (c) Figure 1. (a): Waveforms from LIGO sites [2] and their location and sonograms. Figure from htt s:!!losc.ligo.org!events!GW150914/. 'he gravitational()ave event GW150914 o*served *+ the LIGO ,anford (H1, left column anels) and Livingston (L1, right column anels) detectors. 'imes are sho)n relative to 14 .e tem*er 2015 at 09:#$:45 /'0. For visualization- all time series are 2ltered )ith a 35–350 ,1 *and- ass 2lter to su ress large 5uctuations outside the detectors6 most sensitive fre7uency *and, and *and-re8ect 2lters to remove the strong instrumental s ectral lines. (b): 0hir ing . arro) (S izella asserina) song: fre7uency versus time (in seconds), sho)ing a song made u of a series of chir s. (c): 9 :i istrelle *at call for echolocation. Bats use ultrasound for “seeing” and for social calls. 'his s ectrogram is a graphic re resentation of fre7uencies against time. 'he color re resents the loudness of each fre7uency. 'his s ectrogram sho)s a falling call- )hich *ecomes a steady note. 'he +ello) and green *lotches are noise. 'his is nearl+ a time reverse of *lack hole merger sonograms. ?arco is a mem*er of a team of 3$ h+sicists )or>ing in ,anover- anal+zing data from ,anford and Livingston. ?arco6s dut+ is to *e a)are of and anal+ze the occurrence of an “event= that records the assage of a gravitational )ave, in one of the four lines that automaticall+ trac> the signals from the detectors in the t)o LIGO o*servatories on the other side of the Atlantic. ?arco noticed that the t)o graphs )ere almost identical- des ite having *een registered independentl+ in sites separated *+ "%$$ >m (see Figure 1a)@ for com arison )e include sonograms from animals (see Figures "* and 1c). 'he time that elapsed *et)een the t)o signals diAered *+ about 7 milliseconds. 'hese almost simultaneous records of signals coming from sites far a)a+ from each other- the similarit+ of their shapes and their large size, could not *e an+thing *ut- either: a ossi*le record of a gravitational )ave traveling at the s eed of light or- a “signal= arti2ciall+ “in8ected= to the detectors *+ one of the four mem*ers of the LIGO rogram )ho are allo)ed to “in8ect= dumm+ signals. 'he reason )h+ arti2cial signals are in8ected to the s+stem is to the test )hether the o eration of the detectors is correct and if the dut+ o*servers are able to identif+ a real signal. Follo)ing the re-established rotocols- ?arco tried to verif+ )hether the signals )ere real or the “event= was 8ust a dumm+ in8ected signal. .ince aLIGO was still in engineering mode, there was no )a+ to in8ect fake signals- i.e., hard)are in8ections. 'herefore, ever+one )as nearl+ "$$C certain that this was a detection. ,o)ever- it )as necessar+ to go through the protocols of ma>ing sure that this was the case. ?arco as>ed 9ndre) Lundgren- another ostdoc at ,anover- to 2nd out if the latter )as the case. 9ndre) found no evidence of a “dumm+ in8ection.= On the other hand- the t)o signals detected )ere so clear- the+ did not need to *e 2ltered to remove *ac>ground noise. 'he+ )ere o*vious. ?arco and 9ndre) immediatel+ honed the control rooms at Livingston and ,anford. It )as earl+ morning in the /nited .tates and onl+ someone from Livingston res onded. 'here )as nothing unusual to report. Finall+- one hour after receiving the signal- ?arco sent an e-mail to all collaborators of LIGO as>ing if an+one )as a)are of something that might cause a s urious signal. Do one ans)ered the e-mail. Ea+s later- LIGO leaders sent a report stating that there had not *een an+ “arti2cial in8ection.= ;+ then the news had alread+ *een lea>ed to some other mem*ers of the )orld communit+ of astro h+sicists. Finall+ after several months- the oFcial ne)s of the detection of gravitational )aves )as given at a ress conference on "" Februar+ 2016, after the team had ascertained that the signals )ere not the result of some eH erimental failure, or an+ signal locall+ roduced- earthquake, or electromagnetic 5uctuation. 'his announcement is the most im ortant scienti2c ne)s so far this centur+. Gravitational )aves )ere detected after G$ +ears of searching and "$$ +ears since the rediction of their eHistence. 'he scienti2c aper )as u*lished in Physical Review Letters [2]. 'his discover+ not onl+ con2rmed one of the most *asic redictions of General Ielativit+ *ut also o ened a ne) )indo) of o*servation of the universe, and )e affirm )ithout eHaggeration that a ne) era in astronom+ has been born. In )hat follo)s )e shall narrate the 8ourne+ ex erienced in search of gravitational )aves- including their conception in the earl+ t)entieth centur+- their rediction *+ Jinstein in "%"G- the theoretical controvers+- efforts to)ards detection, and the recent discover+. 2. Lost and Found Gravitational Waves On # Kul+ "%$# the Comptes Rendus of the French Academy of Sciences u*lished an article )ritten *+ ,enri :oincare entitled <.ur la d+namique d6 l6électron.= 'his )or> summarized his theor+ of relativit+ [3]. The wor> ro osed that gravit+ )as transmitted through a )ave that :oincaré called a gravitational wave (onde gravifique). It )ould ta>e some +ears for 9l*ert Jinstein to ostulate in "%"# in 2nal form the 'heor+ of General Ielativit+ [&]. ,is theor+ can *e seen as an eHtension of the . ecial 'heor+ of Ielativit+ ostulated *+ him "$ +ears earlier in "%$# [5]. 'he General 'heor+ eH lains the henomenon of gravit+. In this theor+- gravit+ is not a force—a diAerence from De)ton6s La)M*ut a manifestation of the curvature of s ace–time, this curvature *eing caused *+ the resence of mass (and also energ+ and momentum of an o*8ect). In other )ords- Jinstein6s equations match- on the one side, the curvature of local s ace–time )ith- on the other side of the equation- local energ+ and momentum within that s ace–time. Jinstein6s equations are too com licated to *e solved in full generalit+ and onl+ a fe) ver+ s eci2c solutions that descri*e s ace–times with ver+ restrictive conditions of s+mmetr+ are kno)n. Onl+ )ith such restrictions it is ossi*le to sim lif+ Jinstein6s equations and so 2nd eHact anal+tical solutions. For other cases one must make some sim li2cations or ap roHimations that allo) a solution- or there are cases )here equations can *e solved numericall+ using com uters- )ith advanced techniques in the field called Numerical Relativit+. .hortl+ after having 2nished his theor+ Jinstein con8ectured- 8ust as :oincarL had done, that there could *e gravitational )aves similar to electromagnetic )aves. 'he latter are roduced *+ accelerations of electric charges. In the electromagnetic case, )hat is commonl+ found is di olar radiation roduced b+ s)inging an electric di ole. An electric di ole is formed b+ t)o ( ositive and negative) charges that are separated *+ some distance. Oscillations of the di ole separation generate electromagnetic )aves.
Recommended publications
  • Gravitational Waves: First Joint LIGO-Virgo Detection
    PRESS RELEASE I PARIS I 27 SEPTEMBER 2017 Gravitational waves: first joint LIGO-Virgo detection Scientists in the LIGO and Virgo collaborations have achieved the first ever three-detector observation of the gravitational waves emitted by the merger of two black holes. This is the first signal detected by the Advanced Virgo instrument, which joined observing runs by the two LIGO detectors on 1 August, and confirms that it is fully operational. It opens the way to considerably more accurate localization of the sources of gravitational waves. The discovery is published by the international collaboration that runs the three detectors, including teams from the CNRS, in the journal Physical Review Letters. The announcement was made at a press briefing during a meeting of the G7-science1 in Turin, Italy. On the very same day, the CNRS awarded two Gold Medals to physicists Alain Brillet and Thibault Damour for their major contributions to the detection of gravitational waves2. Black holes are the final stage in the evolution of the most massive stars. Some black holes form a pair, orbiting around each other and gradually getting closer while losing energy in the form of gravitational waves, until a point is reached where the process suddenly accelerates. They then end up coalescing into a single black hole. Merging black holes have already been observed three times by the LIGO detectors, in 2015 and early 20173. This time, three instruments detected the event on 14 August 2017 at 10:30 UTC, enabling vastly improved localization in the sky. This new event confirms that pairs of black holes are relatively common, and will contribute towards the study of such objects.
    [Show full text]
  • Measurement of the Speed of Gravity
    Measurement of the Speed of Gravity Yin Zhu Agriculture Department of Hubei Province, Wuhan, China Abstract From the Liénard-Wiechert potential in both the gravitational field and the electromagnetic field, it is shown that the speed of propagation of the gravitational field (waves) can be tested by comparing the measured speed of gravitational force with the measured speed of Coulomb force. PACS: 04.20.Cv; 04.30.Nk; 04.80.Cc Fomalont and Kopeikin [1] in 2002 claimed that to 20% accuracy they confirmed that the speed of gravity is equal to the speed of light in vacuum. Their work was immediately contradicted by Will [2] and other several physicists. [3-7] Fomalont and Kopeikin [1] accepted that their measurement is not sufficiently accurate to detect terms of order , which can experimentally distinguish Kopeikin interpretation from Will interpretation. Fomalont et al [8] reported their measurements in 2009 and claimed that these measurements are more accurate than the 2002 VLBA experiment [1], but did not point out whether the terms of order have been detected. Within the post-Newtonian framework, several metric theories have studied the radiation and propagation of gravitational waves. [9] For example, in the Rosen bi-metric theory, [10] the difference between the speed of gravity and the speed of light could be tested by comparing the arrival times of a gravitational wave and an electromagnetic wave from the same event: a supernova. Hulse and Taylor [11] showed the indirect evidence for gravitational radiation. However, the gravitational waves themselves have not yet been detected directly. [12] In electrodynamics the speed of electromagnetic waves appears in Maxwell equations as c = √휇0휀0, no such constant appears in any theory of gravity.
    [Show full text]
  • Of the American Mathematical Society August 2017 Volume 64, Number 7
    ISSN 0002-9920 (print) ISSN 1088-9477 (online) of the American Mathematical Society August 2017 Volume 64, Number 7 The Mathematics of Gravitational Waves: A Two-Part Feature page 684 The Travel Ban: Affected Mathematicians Tell Their Stories page 678 The Global Math Project: Uplifting Mathematics for All page 712 2015–2016 Doctoral Degrees Conferred page 727 Gravitational waves are produced by black holes spiraling inward (see page 674). American Mathematical Society LEARNING ® MEDIA MATHSCINET ONLINE RESOURCES MATHEMATICS WASHINGTON, DC CONFERENCES MATHEMATICAL INCLUSION REVIEWS STUDENTS MENTORING PROFESSION GRAD PUBLISHING STUDENTS OUTREACH TOOLS EMPLOYMENT MATH VISUALIZATIONS EXCLUSION TEACHING CAREERS MATH STEM ART REVIEWS MEETINGS FUNDING WORKSHOPS BOOKS EDUCATION MATH ADVOCACY NETWORKING DIVERSITY blogs.ams.org Notices of the American Mathematical Society August 2017 FEATURED 684684 718 26 678 Gravitational Waves The Graduate Student The Travel Ban: Affected Introduction Section Mathematicians Tell Their by Christina Sormani Karen E. Smith Interview Stories How the Green Light was Given for by Laure Flapan Gravitational Wave Research by Alexander Diaz-Lopez, Allyn by C. Denson Hill and Paweł Nurowski WHAT IS...a CR Submanifold? Jackson, and Stephen Kennedy by Phillip S. Harrington and Andrew Gravitational Waves and Their Raich Mathematics by Lydia Bieri, David Garfinkle, and Nicolás Yunes This season of the Perseid meteor shower August 12 and the third sighting in June make our cover feature on the discovery of gravitational waves
    [Show full text]
  • Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
    Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas.
    [Show full text]
  • Einstein's Mistakes
    Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous.
    [Show full text]
  • LIGO Detector and Hardware Introduction
    LIGO Detector and Hardware Introduction Virtual Open Data Workshop May 2020 LIGO-G2000795 Outline • Introduction 45W • Interferometry 40W 1.6kW 200kW Locking Optical cavities • Hardware • Noise Fundamental Technical • Commissioning/Observation Runs • Future Detector Plans • Bibliography Gravitational Waves • Metric tensor perturbation in GR = + 2 polarization in GR Scalar and other possible waves ℎ • Free falling masses • Change in laser propagation time • Phase difference in light ∝ ℎ • Interferometry detects phase difference ∝ ℎ • Astronomical Sources Modeling Modeled Unmodeled /Length Modeled vs Unmodeled Short Inspirals (BBH, Bursts Short vs Long BNS, BH/NS) (Supernova) Long Continuous Waves Stochastic Known vs Unknown (Pulsars) Background Sensitivity Estimate • Strain from single photon: = 10 2 • Need strain 10 � −10 ℎ ≅ • Shot noise SNR− 22 = 10 improvement,∝ � 10 photons At1 1002 Hz equivalent to power24 of 20 MW • • With 200 W of input laser power, 45W 200kW 40W 1.6kW requires power gain of 100,000 Total optical gain in LIGO is ~50,000 Ignores other noise sources Gravitational Wave Detector Network GEO 600: Germany Virgo: Italy KAGRA: Japan Interferometry • Book by Peter Saulson • Michelson interferometer Fringe splitting • Fabry-Perot arms Cavity pole, = ⁄4ℱ • Pound-Drever-Hall locking 45W 200kW 40W 1.6kW Match laser frequency to cavity length RF modulation with EOM • Feedback and controls Other LIGO Cavities • Mode cleaners Input and output 45W 200kW 40W 1.6kW Single Gauss-Laguerre mode • Power recycling Output dark
    [Show full text]
  • Nobel Laureates Endorse Joe Biden
    Nobel Laureates endorse Joe Biden 81 American Nobel Laureates in Physics, Chemistry, and Medicine have signed this letter to express their support for former Vice President Joe Biden in the 2020 election for President of the United States. At no time in our nation’s history has there been a greater need for our leaders to appreciate the value of science in formulating public policy. During his long record of public service, Joe Biden has consistently demonstrated his willingness to listen to experts, his understanding of the value of international collaboration in research, and his respect for the contribution that immigrants make to the intellectual life of our country. As American citizens and as scientists, we wholeheartedly endorse Joe Biden for President. Name Category Prize Year Peter Agre Chemistry 2003 Sidney Altman Chemistry 1989 Frances H. Arnold Chemistry 2018 Paul Berg Chemistry 1980 Thomas R. Cech Chemistry 1989 Martin Chalfie Chemistry 2008 Elias James Corey Chemistry 1990 Joachim Frank Chemistry 2017 Walter Gilbert Chemistry 1980 John B. Goodenough Chemistry 2019 Alan Heeger Chemistry 2000 Dudley R. Herschbach Chemistry 1986 Roald Hoffmann Chemistry 1981 Brian K. Kobilka Chemistry 2012 Roger D. Kornberg Chemistry 2006 Robert J. Lefkowitz Chemistry 2012 Roderick MacKinnon Chemistry 2003 Paul L. Modrich Chemistry 2015 William E. Moerner Chemistry 2014 Mario J. Molina Chemistry 1995 Richard R. Schrock Chemistry 2005 K. Barry Sharpless Chemistry 2001 Sir James Fraser Stoddart Chemistry 2016 M. Stanley Whittingham Chemistry 2019 James P. Allison Medicine 2018 Richard Axel Medicine 2004 David Baltimore Medicine 1975 J. Michael Bishop Medicine 1989 Elizabeth H. Blackburn Medicine 2009 Michael S.
    [Show full text]
  • Ripples in Spacetime
    editorial Ripples in spacetime The 2017 Nobel prize in Physics has been awarded to Rainer Weiss, Barry C. Barish and Kip S. Thorne “for decisive contributions to the LIGO detector and the observation of gravitational waves”. It is, frankly, difficult to find something original to say about the detection of gravitational waves that hasn’t been said already. The technological feat of measuring fluctuations in the fabric of spacetime less than one-thousandth the width of an atomic nucleus is quite simply astonishing. The scientific achievement represented by the confirmation of a century-old prediction by Albert Einstein is unique. And the collaborative effort that made the discovery possible — the Laser Interferometer Gravitational-Wave Observatory (LIGO) — is inspiring. Adapted from Phys. Rev. Lett. 116, 061102 (2016), under Creative Commons Licence. Rainer Weiss and Kip Thorne were, along with the late Ronald Drever, founders of the project that eventually became known Barry Barish, who was the director Last month we received a spectacular as LIGO. In the 1960s, Thorne, a black hole of LIGO from 1997 to 2005, is widely demonstration that talk of a new era expert, had come to believe that his objects of credited with transforming it into a ‘big of gravitational astronomy was no interest should be detectable as gravitational physics’ collaboration, and providing the exaggeration. Cued by detections at LIGO waves. Separately, and inspired by previous organizational structure required to ensure and Virgo, an interferometer based in Pisa, proposals, Weiss came up with the first it worked. Of course, the passion, skill and Italy, more than 70 teams of researchers calculations detailing how an interferometer dedication of the thousand or so scientists working at different telescopes around could be used to detect them in 1972.
    [Show full text]
  • Status of Advanced Virgo
    EPJ Web of Conferences will be set by the publisher EPJDOI: Web will of beConferences set by the publisher182, 02003 (2018) https://doi.org/10.1051/epjconf/201818202003 ICNFPc Owned 2017 by the authors, published by EDP Sciences, 2017 Status of Advanced Virgo F. Acernese51,17, T. Adams26, K. Agatsuma31, L. Aiello10,16, A. Allocca47,21,,a A. Amato28, S. Antier25, N. Arnaud25,8, S. Ascenzi50,23, P. Astone22, P. Bacon1, M. K. M. Bader31, F. Baldaccini46,20, G. Ballardin8, F. Barone51,17, M. Barsuglia1, D. Barta34, A. Basti47,21, M. Bawaj38,20, M. Bazzan44,18, M. Bejger5, I. Belahcene25, D. Bersanetti15, A. Bertolini31, M. Bitossi8,21, M. A. Bizouard25, S. Bloemen33, M. Boer2, G. Bogaert2, F. Bondu48, R. Bonnand26, B. A. Boom31, V. Boschi8,21, Y. Bouffanais1, A. Bozzi8, C. Bradaschia21, M. Branchesi10,16, T. Briant27, A. Brillet2, V. Brisson25, T. Bulik3, H. J. Bulten36,31, D. Buskulic26, C. Buy1, G. Cagnoli28,42, E. Calloni43,17, M. Canepa39,15, P. Canizares33, E. Capocasa1, F. Carbognani8, J. Casanueva Diaz21, C. Casentini50,23, S. Caudill31, F. Cavalier25, R. Cavalieri8, G. Cella21, P. Cerdá-Durán55, G. Cerretani47,21, E. Cesarini6,23, E. Chassande-Mottin1, A. Chincarini15, A. Chiummo8, N. Christensen2, S. Chua27, G. Ciani44,18, R. Ciolfi13,24, A. Cirone39,15, F. Cleva2, E. Coccia10,16, P.-F. Cohadon27, D. Cohen25, A. Colla49,22, L. Conti18, I. Cordero-Carrión56, S. Cortese8, J.-P. Coulon2, E. Cuoco8, S. D’Antonio23, V. Dattilo8, M. Davier25, C. De Rossi28,8, J. Degallaix28, M. De Laurentis10,17, S. Deléglise27, W. Del Pozzo47,21, R. De Pietri45,19, R.
    [Show full text]
  • Joseph Weber's Contribution to Gravitational Waves and Neutrinos
    Firenze University Press www.fupress.com/substantia Historical Article New Astronomical Observations: Joseph Weber’s Contribution to Gravitational Waves Citation: S. Gottardo (2017) New Astronomical Observations: Joseph and Neutrinos Detection Weber’s Contribution to Gravitational Waves and Neutrinos Detection. Sub- stantia 1(1): 61-67. doi: 10.13128/Sub- stantia-13 Stefano Gottardo Copyright: © 2017 S. Gottardo.This European Laboratory for Nonlinear Spectroscopy (LENS), 50019 Sesto Fiorentino (Flor- is an open access, peer-reviewed arti- ence), Italy cle published by Firenze University E-mail: [email protected] Press (http://www.fupress.com/substan- tia) and distribuited under distributed under the terms of the Creative Com- Abstract. Joseph Weber, form Maryland University, was a pioneer in the experimen- mons Attribution License, which per- tal research of gravitational waves and neutrinos. Today these two techniques are very mits unrestricted use, distribution, and promising for astronomical observation, since will allow to observe astrophysical phe- reproduction in any medium, provided nomena under a new light. We review here almost 30 years of Weber’s career spent the original author and source are on gravity waves and neutrinos; Weber’s experimental results were strongly criticized credited. by the international community, but his research, despite critics, boosted the brand Data Availability Statement: All rel- new (in mid-sixties of last century) research field of gravity waves to become one of evant data are within the paper and its the most important in XXI century. On neutrino side, he found an unorthodox way Supporting Information files. to reduce the size of detectors typically huge and he claimed to observe neutrinos flux with a small pure crystal of sapphire.
    [Show full text]
  • Could Minkowski Have Discovered the Cause of Gravitation Before Einstein?
    2 Could Minkowski have discovered the cause of gravitation before Einstein? Vesselin Petkov Abstract There are two reasons for asking such an apparently unanswer- able question. First, Max Born’s recollections of what Minkowski had told him about his research on the physical meaning of the Lorentz transformations and the fact that Minkowski had created the full-blown four-dimensional mathematical formalism of space- time physics before the end of 1907 (which could have been highly improbable if Minkowski had not been developing his own ideas), both indicate that Minkowski might have arrived at the notion of spacetime independently of Poincaré (who saw it as nothing more than a mathematical space) and at a deeper understanding of the basic ideas of special relativity (which Einstein merely postulated) independently of Einstein. So, had he lived longer, Minkowski might have employed successfully his program of regarding four- dimensional physics as spacetime geometry to gravitation as well. Moreover, Hilbert (Minkowski’s closest colleague and friend) had derived the equations of general relativity simultaneously with Ein- stein. Second, even if Einstein had arrived at what is today called Einstein’s general relativity before Minkowski, Minkowski would have certainly reformulated it in terms of his program of geometriz- ing physics and might have represented gravitation fully as the man- ifestation of the non-Euclidean geometry of spacetime (Einstein re- garded the geometrical representation of gravitation as pure math- ematics) exactly like he reformulated Einstein’s special relativity in terms of spacetime. 1 Introduction On January 12, 1909, only several months after his Cologne lecture Space and Time [1], at the age of 44 Hermann Minkowski untimely left this world.
    [Show full text]
  • Ligo-India Proposal for an Interferometric Gravitational-Wave Observatory
    LIGO-INDIA PROPOSAL FOR AN INTERFEROMETRIC GRAVITATIONAL-WAVE OBSERVATORY IndIGO Indian Initiative in Gravitational-wave Observations PROPOSAL FOR LIGO-INDIA !"#!$ Indian Initiative in Gravitational wave Observations http://www.gw-indigo.org II Title of the Project LIGO-INDIA Proposal of the Consortium for INDIAN INITIATIVE IN GRAVITATIONAL WAVE OBSERVATIONS IndIGO to Department of Atomic Energy & Department of Science and Technology Government of India IndIGO Consortium Institutions Chennai Mathematical Institute IISER, Kolkata IISER, Pune IISER, Thiruvananthapuram IIT Madras, Chennai IIT, Kanpur IPR, Bhatt IUCAA, Pune RRCAT, Indore University of Delhi (UD), Delhi Principal Leads Bala Iyer (RRI), Chair, IndIGO Consortium Council Tarun Souradeep (IUCAA), Spokesperson, IndIGO Consortium Council C.S. Unnikrishnan (TIFR), Coordinator Experiments, IndIGO Consortium Council Sanjeev Dhurandhar (IUCAA), Science Advisor, IndIGO Consortium Council Sendhil Raja (RRCAT) Ajai Kumar (IPR) Anand Sengupta(UD) 10 November 2011 PROPOSAL FOR LIGO-INDIA II PROPOSAL FOR LIGO-INDIA LIGO-India EXECUTIVE SUMMARY III PROPOSAL FOR LIGO-INDIA IV PROPOSAL FOR LIGO-INDIA This proposal by the IndIGO consortium is for the construction and subsequent 10- year operation of an advanced interferometric gravitational wave detector in India called LIGO-India under an international collaboration with Laser Interferometer Gravitational–wave Observatory (LIGO) Laboratory, USA. The detector is a 4-km arm-length Michelson Interferometer with Fabry-Perot enhancement arms, and aims to detect fractional changes in the arm-length smaller than 10-23 Hz-1/2 . The task of constructing this very sophisticated detector at the limits of present day technology is facilitated by the amazing opportunity offered by the LIGO Laboratory and its international partners to provide the complete design and all the key components required to build the detector as part of the collaboration.
    [Show full text]