A Numerical Approach to Black Hole Physics
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This project in gravitational physics will apply numerical                 techniques to investigate three dimensional fluid dynamics near                 black holes.  Of special interest will be the development of                    nonaxisymmetric instabilities that threaten black holes                         accretion disks.  Also of interest will be the effects of                       "frame dragging" by rotating black holes.  The effects of                       magnetic fields will be included.
{'FirstName': 'John', 'LastName': 'Hawley', 'PI_MID_INIT': 'F', 'PI_SUFX_NAME': None, 'PI_FULL_NAME': 'John F Hawley', 'EmailAddress': 'jh8h@virginia.edu', 'NSF_ID': '000410349', 'StartDate': '07/01/1988', 'EndDate': None, 'RoleCode': 'Principal Investigator'}
{'Name': 'University of Virginia Main Campus', 'CityName': 'CHARLOTTESVILLE', 'ZipCode': '229034833', 'PhoneNumber': '4349244270', 'StreetAddress': '1001 EMMET ST N', 'StreetAddress2': None, 'CountryName': 'United States', 'StateName': 'Virginia', 'StateCode': 'VA', 'CONGRESSDISTRICT': '05', 'CONGRESS_DISTRICT_ORG': 'VA05', 'ORG_UEI_NUM': 'JJG6HU8PA4S5', 'ORG_LGL_BUS_NAME': 'RECTOR & VISITORS OF THE UNIVERSITY OF VIRGINIA', 'ORG_PRNT_UEI_NUM': None}
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{'Code': '1244', 'Text': 'Gravity Theory'}
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