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Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z The search for gravitational waves Marco Cavaglià Department of Physics and Astronomy University.

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Presentation on theme: "Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z The search for gravitational waves Marco Cavaglià Department of Physics and Astronomy University."— Presentation transcript:

1 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z The search for gravitational waves Marco Cavaglià Department of Physics and Astronomy University of Mississippi LIGO Scientific Collaboration Background picture from http://cgwp.gravity.psu.edu

2 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z What is a gravitational wave?

3 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z A gravitational wave is: …OK, I’ll try to keep it simple!

4 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z A gravitational wave is a propagating disturbance of the spacetime When masses move rapidly, the spacetime becomes stirred by their motion: ripples start travelling outward with the speed of light Einstein’s General Relativity The spacetime geometry is continuously distorted by the presence of mass (=energy).

5 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z What is the effect of a gravitational wave? We will experiment on a graduate student (Mr. Jun-Qi Guo)

6 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Sources of gravitational waves ♦ Coalescing binary neutron stars or black holes ♦ Spinning neutron stars ♦ Gravitational bursts (e.g. supernovae) ♦ Big bang gravitational echo

7 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Sources of gravitational waves ♦ Coalescing binary neutron stars or black holes Picture credit: NASA/CXC/AIfA; NRAO/VLA/NRL ♦ Spinning neutron stars ♦ Gravitational bursts (e.g. supernovae) ♦ Big bang gravitational echo

8 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Sources of gravitational waves ♦ Coalescing binary neutron stars or black holes ♦ Spinning neutron stars ♦ Gravitational bursts (e.g. supernovae) ♦ Big bang gravitational echo Picture credit: NASA/HST/STScI

9 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Sources of gravitational waves ♦ Coalescing binary neutron stars or black holes Picture credit: NASA/HST/STScI ♦ Spinning neutron stars ♦ Gravitational bursts (e.g. supernovae) ♦ Big bang gravitational echo

10 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Sources of gravitational waves ♦ Coalescing binary neutron stars or black holes Picture credit: NASA/WMAP ♦ Spinning neutron stars ♦ Gravitational bursts (e.g. supernovae) ♦ Big bang gravitational echo

11 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z How do we know that gravitational waves exist? John Rowe Animation/Australia Telescope National Facility, CSIRO Indirect detection: slow down of a binary pulsar R. HulseJ. Taylor

12 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z (Picture credit: L. Rezzolla, Albert-Einstein Institute, Golm, Germany) Merger of a binary black hole system (equal-mass, unequal-spin black holes)

13 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z (Courtesy of L. Rezzolla, Albert-Einstein Institute, Golm, Germany) Merger of a binary black hole system (equal-mass, zero-spin black holes)

14 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z What is LIGO?

15 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z A way to answer is to use the most incredible scientific tool of the new millennium:

16 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Input Beam (Laser) RM BSBS ITMX ITMY ETMY ETMX Reflected Port Anti-Symmetric Port Pickoff Port LyLy LxLx Strain Readout (L y -L x ) 6 W 250 W 14 kW ~0.2 W LIGO is an interferometer

17 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Livingston (LA) 4 km interferometer Hanford (WA) 4 km + 2 km interferometers The LIGO Observatory

18 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z

19 Livingston, Louisiana

20 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Vacuum equipment

21 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Core optic suspensions

22 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Core optics

23 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z The control room Vitor Cardoso

24 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Science Requirement. document (1995) S2: Feb.- Apr. 2003 59 days BNS reach ~ 1Mpc S3: Oct. ‘03 - Jan. ‘04 70 days BNS reach ~ 3Mpc S5: Nov 2005 – Current S4: Feb. - Mar. 2005 30 days BNS reach ~ 15Mpc LIGO sensitivity Distance Earth-Sun (93.2 million miles)… …stretches by a fraction of an atom!

25 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z LIGO is so sensitive that it feels… ♦ Cars and trucks ♦ Airplanes ♦ Sea waves ♦ Earthquakes…

26 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Australian Consortium for Interferometric Gravitational Astronomy The Univ. of Adelaide Andrews University The Australian National Univ. The University of Birmingham California Inst. of Technology Cardiff University Carleton College Charles Stuart Univ. Columbia University Embry Riddle Aeronautical Univ. Eötvös Loránd University University of Florida German/British Collaboration for the Detection of Gravitational Waves University of Glasgow Goddard Space Flight Center Leibniz Universität Hannover Hobart & William Smith Colleges Inst. of Applied Physics of the Russian Academy of Sciences Polish Academy of Sciences India Inter-University Centre for Astronomy and Astrophysics Louisiana State University Louisiana Tech University Loyola University New Orleans University of Maryland Max Planck Inst. for Gravitational Physics University of Michigan University of Minnesota The University of Mississippi Massachusetts Inst. of Technology Monash University Montana State University Moscow State University National Astronomical Observatory of Japan Northwestern University University of Oregon Pennsylvania State University Rochester Inst. of Technology Rutherford Appleton Lab University of Rochester San Jose State University Univ. of Sannio at Benevento, and Univ. of Salerno University of Sheffield University of Southampton Southeastern Louisiana Univ. Southern Univ. and A&M College Stanford University University of Strathclyde Syracuse University Univ. of Texas at Austin Univ. of Texas at Brownsville Trinity University Universitat de les Illes Balears Univ. of Massachusetts Amherst University of Western Australia Univ. of Wisconsin-Milwaukee Washington State University University of Washington

27 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z You can also contribute!

28 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z The Einstein@home Project http://www.einsteinathome.org Sat Sept 8 2007 19:44 UTC

29 Liberal Arts Faculty Forum – Sept. 18th, 2007 LIGO-G070613-00-Z Thank you!


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