'Bh bh' presentation slideshows

Cosmological Heavy Ion Collisions: Colliding Neutron Stars and Black Holes

HIM@Korea.U. Current Status of Numerical Approaches. Cosmological Heavy Ion Collisions: Colliding Neutron Stars and Black Holes. Chang-Hwan Lee. Introduction. EM wave Theory: Maxwell (1873) Acceleration of electric charge Detection : H. Hertz (1888). Grav. wave

666 views • 59 slides

Current status of numerical relativity Gravitational waves from coalescing compact binaries

Current status of numerical relativity Gravitational waves from coalescing compact binaries. Masaru Shibata (Yukawa Institute, Kyoto University). GW spectrum from compact binaries. Initial LIGO. Chirp. h=h ( f ) f. Merge. Prediction only by

412 views • 31 slides

LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology LIGO PAC Meeting Pasadena, 5 June 2003 LIGO-G030293-00-R. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

350 views • 20 slides

ASTROPHYSICS

ASTROPHYSICS. Kip S. Thorne CaRT, California Institute of Technology NSF Advanced LIGO Review Pasadena, 11 June 2003. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate. Most Pessimistic

330 views • 20 slides

Merger phase simulations of binary-systems: status

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Merger phase simulations of binary-systems: status

302 views • 19 slides

LIGO SCIENCE

LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF LIGO Operations Panel Hanford - 26 February 2001. LIGO-G010183-00-M. 300 in h ~10 7 in rate. Most Optimistic Source Strengths. h rms = h(f) ?f ~ 10 h(f). Open up wider band. 15 in h ~3000 in rate.

292 views • 18 slides

ADVANCED LIGO SCIENCE

ADVANCED LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF Advanced R&D Panel - 29 January 2001. 300 in h ~10 7 in rate. h rms = h(f) ?f ?10 h(f). Open up wider band. 15 in h ~3000 in rate. From Initial Interferometers to Advanced. Most Optimistic Source

295 views • 17 slides

ADVANCED LIGO SCIENCE

ADVANCED LIGO SCIENCE. Kip S. Thorne CaRT, California Institute of Technology NSF Advanced R&D Panel - 29 January 2001. 300 in h ~10 7 in rate. h rms = h(f) ?f ?10 h(f). Open up wider band. 15 in h ~3000 in rate. From Initial Interferometers to Advanced. Most Optimistic Source

172 views • 17 slides

Dihybrid Crosses

Dihybrid Crosses. Homework. Dihybrid Crosses. Popcorn reading: The first two pages of the handout, telling the story of the Morgan fruit fly experiments. Dihybrid Crosses.

314 views • 16 slides

Population synthesis and binary black hole merger rates

265 views • 16 slides

Compact object merger rates Predictions Constraints (including short GRBs)

229 views • 15 slides

Probability of detecting compact binary coalescence with enhanced LIGO

296 views • 14 slides

Understanding Area Lesson 11.1

Understanding Area Lesson 11.1. Units of measure 1. Linear units: perimeter, circumference 2. Square units: area 3. Cubic units: volume. Definition: The area of a closed region is the number of square units of space within the boundary of the region. Area of a rectangle:

282 views • 12 slides