PPT-LISA in the Gravitational Wave Decade

John W Conklin for the GWSIG University of Florida jwconklinufledu Gravitational Wave Decade LISA ranked 2 nd after WFIRST in NWNH 2030 BICEP 2 2014 aLIGO VIRG0 detection 2020 Decadal. Millisecond . Pulsars:. Dan Stinebring. Oberlin College. CWRU – May 21, 2009. . George Greenstein. (Amherst College). Discovery of “Millisecond” Pulsars. 1982 – Arecibo Observatory – Don Backer, Sri Kulkarni, .... To demonstrate the physical reality of gravitational waves, consider the example system of the previous section. We will concentrate our attention on three of the test masses, one chosen arbitrarily from the plane, along with its nearest neighbors in the +x and +y directions. Imagine that we have equipped the mass at the vertex of this “L” with a lamp that can be made to emit very brief pulses of light. Imagine also that the two masses at the ends of the “L” are fitted with mirrors aimed so that they will return the flashes of light back toward the vertex mass. The Child of General Relativity. A Necessary Change. Concepts after Einstein :-. Time is not absolute. There is no ether frame. Notion of . spacetime. Concepts before Einstein :-. There is a preferred reference frame ether. Sources and detection . Ravi . kumar. . Kopparapu. Center for Gravitational-Wave Physics (CGWP) . Gravity. Einstein’s General theory of relativity :. Gravity is a manifestation of curvature of 4- dimensional (3 space + 1 time) space-time produced by matter (metric equation ? g. (& Gravitons ?). -. Vishal. . Kasliwal. Classical Electromagnetism. Vacuum. Maxwell Field Equations. Light!!. Electromagnetic waves. Quantum Electromagnetism. Hamiltonian of Quantized. Field. where. 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. John Baker, NASA/GSFC. GWADW 2018. Gridwood, AK - 13 May 2018. LISA: Opening the millihertz band. ‹#›. . . Numerous sources. . . Stronger gravity. LISA science in milli-Hz band. Science Objectives:. Mission Concept Study. Robin Stebbins, Study Scientist. Ninth LISA Symposium. Paris, 22 May 2012. Outline. Goals. Elements of the study. Context of the study. Responses to the Request-For-Information (RFI). (SGO)-. Mid. Minimum. . Cost 3-arm/6-link. LISA-like Mission. Presented by Jeff . Livas. for . the SGO Core Team. Concept Description. Rationale for the configuration. Try to find lowest . cost 6 . Ra Inta (Texas Tech University) . for the LIGO Scientific Collaboration and the Virgo . Collaboration. LIGO . Document . G1700692-v3. 1. A tour of some applied mathematical tools used within the LIGO and Virgo collaborations. 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 UsingdatatakenbetweenNovember2005and2007theLaserInterferometerGravitational-waveObservatoryLIGOScientificCollaborationandtheVirgoCollaborationhaveplacedupperlimitsontheamplitudeofthestochasticgravitat 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;.