PPT-The Laser Interferometer Space Antenna: Millihertz gravitational wave science

John Baker NASAGSFC GWADW 2018 Gridwood AK 13 May 2018 LISA Opening the millihertz band Numerous sources Stronger gravity LISA science in milliHz band Science Objectives. Benabid M Notcutt L Ju DG Blair Physics Department University of Western Australia Nedlands WA 6907 Australia Abstract We report measurements of the birefringence of a high purity polished sapphire sample to determine the fringe contrast attainable InSpRL. ). Dec-21-2011. Workshop on Gravity Wave Detection . Presenter: Babak . N . Saif. InSpRL. Team. . Gravitational-Wave Mission RFI . Submitted by: Dr. Babak N. Saif, Instrument PI, GSFC Optics Branch, . Overview of Why and How. Dan Burbank and Tony Young. AST5022. Introduction. Background. Physics. Sources. Detectors and Detector Implications. Questions. Gravitational Waves . Speed-of-light wave propagation solution of Einstein’s Field Equations. Gang Jin,. Yuqiong Li, Yuhui Dong, Heshan Liu, . Ziren Luo. . Institute of Mechanics, Chinese Academy of Science, Beijing, 100190. 10. th. LISA Symposium. Gainesville. , . May 1. 9-. 23, . 201. 4. Segment Optics and Space Instruments. 1 . Department of Electrical and Telecommunications Engineering, New York City College of Technology. 2. Instrument Systems and Technology, Optics Division, NASA Goddard Space Flight Center. InSpRL. ). Dec-21-2011. Workshop on Gravity Wave Detection . Presenter: Babak . N . Saif. InSpRL. Team. . Gravitational-Wave Mission RFI . Submitted by: Dr. Babak N. Saif, Instrument PI, GSFC Optics Branch, . Atom . Interferometry. Mark Kasevich. Stanford University. Light-pulse . a. tom interferometers. 2015 laboratory sensor, atomic wavepackets separate by 12 cm before interfering, . 1e-13 . g resolution after 1 hr.. -12 . cm. A world-shaking discovery. James Clerk Maxwell. Professor at King’s College. London: 1860 – 1865. Unified theory of electricity and . . magnetism. Predicted electromagnetic waves. Identified light as due to these waves. https://www.ligo.caltech.edu/system/video_items/files/4/EinsteinsMessengerLIGO.mp4?1436490806. 2017 Nobel Prize in Physics. : Rainer Weiss - Barry C. . Barish. -Kip S. . Thorne. "for . decisive contributions to the LIGO detector and the observation of gravitational waves". NSF and the Laser Interferometer Gravitational - Wave Observatory In 1916 , Albert Einstein published the paper that predicted gravitational waves – ripples in the fabric of space - time resulti e In 1916 Albert Einstein published the collision in unprecedented detail providing insights only entering laser beam into two beams each traveling National Science FoundationLIGO FACTSHEET within 10 milliseconds of one another 150 that indicates a gravitational wave And from that minute change scientists are further able to identify the wave146s source and very broadly where in the univ Tim Kovachy. Department of Physics and Astronomy and Center for Fundamental Physics, Northwestern University. NPS Colloquium. February 1, 2019 . Conceptual overview of atom interferometry. Motivation for gravitational wave detection in the “mid-band” frequency range of ~ 0.1 Hz to 10 Hz. gravitational. . waves. by. Laser-plasma . interaction. . Hedvika . Kadlecová. . a. , . S. Weber . a. , G. Korn. a . a. . Institute of Physics, v.v.i. ASCR, Na Slovance 1999, Prague, Czech Republic;.