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Lars Bildsten
University Of California-Santa Barbara
$59,416,303
Attributed
$79,037,036
Total exposure
11
Grants
11
Lead (contact PI)
Attributed= this PI's even-split share of every grant they're on (the fair, additive number). Exposure = full size of all those grants.
Funding over time
peak $28.2M · FY2006–23$50M$37.5M$25M$12.5M$0
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
NSF$79,037,036 · 11
By mechanism
—$79,037,036 · 11
Top collaborators
- Boris I Shraiman2 shared
- David Gross2 shared
- Leon M Balents2 shared
Grant awards (11)
Kavli Institute for Theoretical Physics$10,064,091
· FY2023 · MPS · contact PI
Kavli Institute for Theoretical Physics$16,096,887
· FY2018 · MPS · contact PI
Collaborative Research: SI2-SSI: Modules for Experiments in Stellar Astrophysics$826,773
· FY2017 · CSE · contact PI
Collaborative Research: SI2-SSE: Modules for Experiments in Stellar Astrophysics$163,586
· FY2014 · CSE · contact PI
Kavli Institute for Theoretical Physics$28,026,478
· FY2012 · MPS · contact PI
Collaborative Research: Modeling Advanced LIGO Gravitational Wave Sources and Their Electromagnetic Counterparts$211,192
· FY2012 · MPS · contact PI
Explosions in White Dwarf Binaries$785,289
· FY2011 · MPS · contact PI
Explosions on Accreting White Dwarfs: From Novae to Supernovae$520,986
· FY2007 · MPS · contact PI
Kavli Institute for Theoretical Physics$22,000,000
· FY2006 · MPS · contact PI
Probing the Deep Interiors of Accreting White Dwarfs through Studies of their Non-Radial Oscillations$309,410
· FY2002 · MPS · contact PI
Pulsations in Rapidly Rotating Main Sequence Stars and Accreting White Dwarfs$32,344
· FY2000 · MPS · contact PI