An award, sponsored by the Division of Gravitational Physics, for best presentation by a student will be made at each of the following annual regional meetings:
- East Coast Gravity Meeting EGM20
- Midwest Relativity Meeting MRM27
- Gulf Coast Gravity Meeting GCGM8
- Pacific Coast Gravity Meeting PCGM34
The award is $200 and gives the recipient the right to advertise her/himself as winning the Division of Gravitational Physics Best Student Presentation at the particular meeting.
Criteria governing the award:
- The only candidates are those who have not yet officially received PhD degrees.
- A member of the Division shall organize the judging of presentations. Judges may include faculty members and postdoctoral associates, but are not to include students.
- The criteria for winning shall be a continuation of the criteria previously used for the award of the Bell prize at Pacific Coast Gravity Meetings. This means, in particular, that the quality of the research and of the presentation will be weighted as the judges see fit.
- The Division member taking responsibility for organizing the judging will notify the Secretary-Treasurer, in advance of the meeting, and will notify the Secretary-Treasurer of the outcome of the judging, including contact information for the winner. The Secretary-Treasurer will then arrange to have the prize money sent to the winner.
- The prize can be split, but this is strongly discouraged.
Congratulations to all of our past winners:
|2017||MWRM27||Katelyn Breivik (Northwestern)||Revealing the Milky Way’s black hole population with Gaia|
|2017||EGM20||Beatrice Bonga (Penn State)||On the Conceptual Confusion in the Notion of Transverse-Traceless Modes|
|Rahul Kashyap (U Mass Dartmouth)||Type Ia Supernovae through Spiral Instability in Binary White Dwarf Mergers|
|2017||PCGM33||Maximiliano Isi (Caltech)||Polarizations of continuous gravitational waves in the advanced detector era|
|2016||MWRM26||Zoheyr Doctor (University of Chicago)||Gravitational Wave Emulation Using Gaussian Process Regression|
|2016||EGM19||Jim Mertens (CWRU)||Computing Observables in an Inhomogeneous Universe using Numerical Relativity|
|2016||PCGM32||Matt Giesler (Caltech)||Nearly extremal binary black hole simulations|
|2015||EGM18||Béatrice Bonga (Penn State)||The quadrupole formula with a positive cosmological constant|
|2015||GCGM8||Hector Okada da Silva (Ole Miss)||A post-TOV formalism for relativistic stars|
|2015||MRM25||Hsin-Yu Chen (University of Chicago)||Optimizing gravitational wave sources followup strategies|
|2014||EGM17||Philippe Landry (Guelph)||Relativistic theory of surficial Love numbers|
|2014||MRM24||Kartik Prabhu (University of Chicago)||Growth rate of black hole instabilities|
|2013||GCGM7||Laleh Sadeghian (WUSTL)||Dark matter distributions around massive black holes: A fully general relativistic approach|
|2013||MRM23||Ben Farr (Northwestern)|
|2012||MRM22||Justin Ellis (UWM)|
|2012||PCGM28||Benson Way (UCSB)||Finite Size Effects in Holographic Superconductors|
|2011||MRM21||Stephen Green (University of Chicago)|
|2010||MRM20||Benjamin Lackey (UWM)|
|2009||MRM19||Sam Gralla (University of Chicago)||Electromagnetic Analog of Binary Black Hole Bobbing and Kicks|
|2008||MRM18||Sam Gralla (University of Chicago)|
|2007||MRM17||Jocelyn Read (UWM)|
|2006||MRM16||Nicolas Yunes (Penn State)||How to Kick a Hole and Other Eccentric Stories|
|2005||PCGM21||Joey Shapiro-Key (Montana State University)||Extending the WMAP Bound on the Size of the Universe|
|2004||PCGM20||Henriette Elvang (UCSB)|
|Louis Rubbo (Montana State University)||Identification and Subtraction of Bright Galactic Binaries from LISA Data|
|2004||MRM14||Ishai Ben-Dov (University of Chicago)|
|2003||MRM13||William Komp (UWM)|
|2003||PCGM19||Henriette Elvang (UCSB)|
|2002||MRM12||Matthew Duez (UIUC)|
|1994||PCGM10||Rhett Herman (Montana State University)||Charged pair production in the Reissner-Nordstrom black hole interior|
If you know of a winner not listed here, please contact us.