Fundamental physics with the laser astrometric test of relativity

Publikation: Beitrag in Buch/Konferenzbericht/Sammelband/GutachtenBeitrag in KonferenzbandBeigetragenBegutachtung

Beitragende

  • S. G. Turyshev - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • H. Dittus - , Universität Bremen (Autor:in)
  • C. Lämmerzahl - , Universität Bremen (Autor:in)
  • S. Theil - , Universität Bremen (Autor:in)
  • W. Ertmer - , Leibniz Universität Hannover (LUH) (Autor:in)
  • E. Rasel - , Leibniz Universität Hannover (LUH) (Autor:in)
  • R. Foerstner - , Airbus Group (Autor:in)
  • U. Johann - , Airbus Group (Autor:in)
  • S. Klioner - , Arbeitsgruppe Astronomie, Lohrmann-Observatorium, Technische Universität Dresden (Autor:in)
  • M. Soffel - , Arbeitsgruppe Astronomie, Lohrmann-Observatorium, Technische Universität Dresden (Autor:in)
  • B. Dachwald - , Deutsches Zentrum für Luft- und Raumfahrt (DLR) e.V. (Autor:in)
  • W. Seboldt - , Deutsches Zentrum für Luft- und Raumfahrt (DLR) e.V. (Autor:in)
  • V. Perlick - , Technische Universität Berlin (Autor:in)
  • M. C.W. Sandford - , Rutherford Appleton Laboratory (Autor:in)
  • R. Bingham - , Rutherford Appleton Laboratory (Autor:in)
  • B. Kent - , Rutherford Appleton Laboratory (Autor:in)
  • T. J. Sumner - , Imperial College London (Autor:in)
  • O. Bertolami - , Universidade de Lisboa (Autor:in)
  • J. Páramos - , Universidade de Lisboa (Autor:in)
  • B. Christophe - , Office national d'études et de recherches aérospatiales (Autor:in)
  • B. Foulon - , Office national d'études et de recherches aérospatiales (Autor:in)
  • P. Touboul - , Office national d'études et de recherches aérospatiales (Autor:in)
  • P. Bouyer - , Institut d'optique Graduate School (Autor:in)
  • T. Damour - , Institut des Hautes Etudes Scientifiques (Autor:in)
  • C. Salomon - , Ecole Normale Superieure (Autor:in)
  • S. Reynaud - , Ecole Normale Superieure (Autor:in)
  • A. Brillet - , Observatoire de la Cote d'Azur (Autor:in)
  • F. Bondu - , Observatoire de la Cote d'Azur (Autor:in)
  • J. F. Mangin - , Observatoire de la Cote d'Azur (Autor:in)
  • E. Samain - , Observatoire de la Cote d'Azur (Autor:in)
  • B. Bertotti - , Università degli Studi di Pavia (Autor:in)
  • L. Iess - , University of Rome La Sapienza (Autor:in)
  • C. Erd - , ESTEC - European Space Research and Technology Centre (Autor:in)
  • J. C. Grenouilleau - , ESTEC - European Space Research and Technology Centre (Autor:in)
  • D. Izzo - , ESTEC - European Space Research and Technology Centre (Autor:in)
  • A. Rathke - , ESTEC - European Space Research and Technology Centre (Autor:in)
  • S. W. Asmar - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • M. Colavita - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • Y. Gürsel - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • H. Hemmati - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • M. Shao - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • J. G. Williams - , Jet Propulsion Laboratory, California Institute of Technology (Autor:in)
  • K. L. Nordtvedt - , Northwest Analysis (Autor:in)
  • I. Shapiro - , Harvard University (Autor:in)
  • R. Reasenberg - , Harvard University (Autor:in)
  • R. W.P. Drever - , California Institute of Technology (Autor:in)
  • J. Degnan - , Sigma Space Corporation (Autor:in)
  • J. E. Plowman - , Montana State University (Autor:in)
  • R. Hellings - , Montana State University (Autor:in)
  • T. W. Murphy - , University of California at San Diego (Autor:in)

Abstract

The Laser Astrometric Test Of Relativity (LATOR) is a European-U.S. Michelson-Morley-type experiment designed to test the tensor metric nature of gravitation - the fundamental postulate of Einstein's theory of general relativity. By using a combination of independent timeseries of highly accurate gravitational deflection of light in the immediate proximity to the Sun along with measurements of the Shapiro time delay on the interplanetary scales (to a precision respectively better than 10-13 radians and 1 cm), LATOR will significantly improve our knowledge of relativistic gravity. The primary mission objective is to i) measure the key post-Newtonian Eddington parameter 7 with accuracy of a part in 109. (1 - γ) is a direct measure for presence of a new interaction in gravitational theory, and, in its search, LATOR goes a factor 30,000 beyond the present best result, Cassini's 2003 test. Other mission objectives include: ii) first measurement of gravity's non-linear effects on light to ∼0.01% accuracy; including both the traditional Eddington β parameter and also the spatial metric's 2nd order potential contribution(never been measured before); iii) direct measurement of the solar quadrupole moment J2 (currently unavailable) to accuracy of a part in 200 of its expected size; iv) direct measurement of the "frame-dragging" effect on light by the Sun's rotational gravitomagnetic field to one percent accuracy. LATOR's primary measurement pushes to unprecedented accuracy the search for cosmologically relevant scalar-tensor theories of gravity by looking for a remnant scalar field in today's solar system. The key element of LATOR is a geometric redundancy provided by the laser ranging and long-baseline optical interferometry. LATOR is envisaged as a partnership between European and US institutions and with clear areas of responsibility between the space agencies: NASA provides the deep space mission components, while optical infrastructure on the ISS is an ESA contribution. We discuss the mission and optical designs of this proposed experiment.

Details

OriginalspracheEnglisch
TitelProceedings of the 39th ESLAB Symposium
Herausgeber (Verlag)European Space Agency
Seiten11-18
Seitenumfang8
Auflage588
ISBN (Print)9290928999, 9789290928997
PublikationsstatusVeröffentlicht - 2005
Peer-Review-StatusJa

Publikationsreihe

ReiheEuropean Space Agency, (Special Publication) ESA SP
Nummer588
ISSN0379-6566

Konferenz

Titel39th ESLAB Symposium: Trends in Space Science and Cosmic Vision 2020
Dauer19 - 21 April 2005
StadtNoordwijk
LandNiederlande

Externe IDs

ORCID /0000-0003-4682-7831/work/168206682

Schlagworte

Schlagwörter

  • Fundamental physics, Laser ranging, LATOR mission, Scalar-tensor theories, Tests of general relativity