EFTA00750374.pdf

From: Jes Staley .cz ill=a> To: mjeevacation@gmail.core <jeevacation@gmail.com> Subject: Fw: Date: Fri, 03 Dec 2010 12:29:08 +0000 Fyi From: To: J Sent: Thu Dec 02 22:48:24 2010 Subject: Fw: ri 1 M I like his research!! Original Message From: Andrew MacFadyen Sender: < Date• Th 2 D 2 10 22:37:03 To: Subject: Re: Dear Thanks for writing. Your message is timely. I and my group at NYU are working on several projects in computational astrophysics, particularly focusing on relativistic gas dynamics and very recently including coupling to dynamical space times. We are very much starting to move into numerical relativity with an eye toward accurate inclusion of gas dynamics relevant for neutron star-black hole and neutron star-neutron star binaries. We are motivated by advanced LIGO which I'm sure you are aware is scheduled to be on line starting in 2014 and is expected to detect double neutron star mergers to 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 mesh refinement on massively parallel computers to simulate black hole mergers at very high resolution. I am on sabbatical at Harvard this coming semester. But I will stay in touch with the application process. Good luck with your application. Best Wishes, Andrew On Thu, Dec 2, 2010 at 10:12 PM, wrote: > Dear Professor MacFayden, > • My name is and I am a senior at Bowoin College in Brunswick, > Maine. I am a physics major and math minor in pursuit of a PhD. in physics. > I am very interested in the physics graduate program at NYU, and will be > submitting my application shortly. > During my time at Bowdoin I have focused on general relativity, and this EFTA00750374 > past summer I conducted research in the field of numerical relativity. More > specifically, 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 in another coordinate system called the "moving puncture" > coordinate, which is now widely used in numerical relativity. I will > continue this research throughout the academic year and my work will > culminate with a thesis paper that I will present to the Physics Department > in the spring. > • I understand that your research is in computational astrophysics, which is a > field that I am interested in. At your convenience, I would love to hear > more about your research. > • Thanks, Andrew MacFadyen New York University http: cosmo.nyu.edu/aim This email is confidential and subject to important disclaimers and conditions including on offers for the purchase or sale of securities, accuracy and completeness of information, viruses, confidentiality, legal privilege, and legal entity disclaimers, available at http://www.jpmorgan.com/pages/disclosures/email. EFTA00750375