Epstein Secrets

several 100 Mpc distances at which the event rate should be sufficient to yield detections. A graduate student in my group has recently written an Einstein/hydro code in 1D to simulate black hole formation during collapse of massive stars. Our goal is to extend this code to 3D using efficient adaptive

y, I created a code in Fortran 90 that simulates the collapse of > a spherically symmetric dust cloud of uniform density and zero pressure into > a Schwarzschild black hole. As you might know, Oppenheimer and Snyder have > an analytical solution to this collapse; my project entails verifying this > collapse

several 100 Mpc distances at which the event rate should be sufficient to yield detections. A graduate student in my group has recently written an Einstein/hydro code in ID to simulate black hole formation during collapse of massive stars. Our goal is to extend this code to 3D using efficient adaptive

y, I created a code in Fortran 90 that simulates the collapse of > a spherically symmetric dust cloud of uniform density and zero pressure into > a Schwarzschild black hole. As you might know, Oppenheimer and Snyder have > an analytical solution to this collapse; my project entails verifying this > collapse

several 100 Mpc distances at which the event rate should be sufficient to yield detections. A graduate student in my group has recently written an Einstein/hydro code in 1D to simulate black hole formation during collapse of massive stars. Our goal is to extend this code to 3D using efficient adaptive

y, I created a code in Fortran 90 that simulates the collapse of > a spherically symmetric dust cloud of uniform density and zero pressure into > a Schwarzschild black hole. As you might know, Oppenheimer and Snyder have > an analytical solution to this collapse; my project entails verifying this > collapse