PPT-LIGO - Fermi Sub-Threshold Search

for the 1 st Advanced LIGO Science Run Jordan Camp NASA Goddard Space Flight Center Moriond Gravitation Meeting March 25 2015 Search Team Lindy Blackburn CfA Nelson Christensen Carleton College. DPF 2015 – University of Michigan, Ann Arbor. . Alejandro Lopez . in collaboration with: C. Savage, D. Spolyar and D. Adams. Outline:. Brief Introduction. Goal. Technique. Results. Conclusion. Future Work. (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters). main . signatures to . be determined: . E. min . , . E. max. [. Ã. timescale . t. acc. (E. ) ], . spectral slope . An Indo-US joint mega-project concept proposal. . IndIGO Consortium. (. Ind. ian . I. nitiative in . G. ravitational-wave . O. bservations). Tarun . Souradeep. IUCAA . (. Spokesperson, IndIGO). CBC (“. inspiral. ”) papers. S1: . Analysis of LIGO data for gravitational waves from binary neutron stars.. Phys. Rev. D . 69. (2004) 122001 . gr-qc/0308069. S2: . Search for gravitational waves from galactic and extra-galactic binary neutron stars.. Who is This Fermi and Why Does He Ask Questions?. . . Fermi questions receive their name from Enrico Fermi (1901-1954). He was an Italian physicist known for his participation in the Los Alamos atomic bomb project (code named the “Manhattan Project”) during World War II. Fermi is best known for his contributions to nuclear physics and the development of quantum theory. In addition to his contribution to theory, he is also noted as an experimentalist.. Fermi National Accelerator Lab December 13, 2017 . How we usually think of him. Or perhaps . l. ike . t. his . How I think of him. There’s a story behind that orange line on the right of the image…... Laser . Interferometer . Gravitational . Wave . Observatory. Hiroaki Yamamoto Caltech/LIGO. Introduction. Newton’s gravity to Einstein’s general relativity. Gravitational Wave. Source and signal. LIGO SURF 2016 Final Presentation. August 18, 2016. Ka-Lok (Rico), Lo. Department of Physics, The Chinese University of Hong Kong. Mentors: . Surabhi. . Sachdev. , Kent Blackburn, and Alan Weinstein. Introduction. Initial LIGO and advanced LIGO. Sensitivities. Commissioning status. Targeting . the first . observations. 1. Some . slides are . from “. ET-. aLIGO. . and . beyond”, LIGO-G14001331, by David Shoemaker. -Style. Peter Couvares. Syracuse . University, LIGO . Scientific . Collaboration. Condor Week 2013. 1 May 2013. Who am I. ? What is LIGO?. Former Condor Team member (‘99-’08).. Now at Syracuse . LIGO is an acronym for Laser Interferometer Gravitational-wave Observatory. The word indistinguishability of the electrons. ,. electron wave nature. ,. the Pauli exclusion principle. .. (4.6). The function . f. (E). called . the . Fermi-Dirac distribution function. gives the probability that an available energy . Peter Couvares. Syracuse University. LIGO Scientific Collaboration. Who am I? What is LIGO?. Former Condor Team member (‘99-’08).. Now at Syracuse University focused on distributed computing problems for the LIGO Scientific Collaboration, and fostering a research computing community at SU more generally.. Jonah Kanner. , Branson Stephens. , . Michele . Vallisneri. , Alan Weinstein, Roy . Williams. 8/11/14. LOSC. 1. LIGO-. G1400509v4. Why LOSC? . Access data with ease. No need to login to LDAS cluster.