Generated by GPT-5-mini| Marc Kamionkowski | |
|---|---|
| Name | Marc Kamionkowski |
| Birth date | 1965 |
| Birth place | New York City |
| Nationality | American |
| Fields | Cosmology, Particle Physics, Astroparticle Physics |
| Workplaces | California Institute of Technology, Johns Hopkins University, Brookhaven National Laboratory, Kavli Institute for Particle Astrophysics and Cosmology |
| Alma mater | Harvard University, Columbia University |
| Doctoral advisor | Lawrence M. Krauss |
Marc Kamionkowski is an American theoretical cosmologist and particle physicist known for work on cosmic microwave background radiation, dark matter, and inflationary cosmology. He has held faculty positions at major research universities and national laboratories and has contributed influential theoretical models and observational predictions that guided experiments in astrophysics and particle physics. His career bridges collaborations with experimental teams and theory groups across institutions and international projects.
Born in New York City, he completed undergraduate studies at Harvard University where he engaged with faculty associated with Steven Weinberg-era quantum field theory and John Bahcall-related astrophysics questions. He pursued graduate studies at Columbia University under the supervision of Lawrence M. Krauss, producing a doctoral thesis that connected early-universe inflationary scenarios with observational signatures sought by teams at NASA and European Space Agency. His formative years included interactions with researchers from Princeton University, Massachusetts Institute of Technology, University of Chicago, and laboratories such as Fermi National Accelerator Laboratory and Brookhaven National Laboratory.
He served on the faculty at Johns Hopkins University before joining the faculty of California Institute of Technology, affiliating with institutes including the Kavli Institute for Particle Astrophysics and Cosmology and collaborating with groups at SLAC National Accelerator Laboratory and Lawrence Berkeley National Laboratory. He has held visiting appointments at institutions such as Stanford University, University of California, Berkeley, and Institute for Advanced Study. He participated in advisory roles for projects led by consortia including BICEP, Planck Collaboration, Simons Observatory, and observatories coordinated with National Science Foundation funding. His career includes interactions with experimental collaborations at South Pole Telescope and partnerships with theorists from University of Cambridge, Oxford University, and Imperial College London.
His theoretical work addressed the imprint of primordial gravitational waves on the polarization of the cosmic microwave background, developing predictions that influenced the design of polarimeters used by teams such as BICEP2 and Planck Collaboration. He contributed to calculations of non-Gaussianity and anisotropies relevant to analyses by researchers at WMAP and ACT (Atacama Cosmology Telescope). In particle astrophysics, he proposed and refined models for weakly interacting massive particles that connected to searches at Large Hadron Collider experiments like ATLAS and CMS, and to direct-detection efforts at facilities such as LUX-ZEPLIN and XENON1T. His work on axion-like particles and sterile neutrinos engaged communities associated with IceCube Neutrino Observatory and Super-Kamiokande. He developed statistical and phenomenological tools used by collaborations at DESI and LSST to interpret large-scale structure and dark-matter halo properties, interfacing with theoretical frameworks emerging from inflationary cosmology and scenarios influenced by concepts from supersymmetry and string theory research. He has published influential reviews connecting theoretical predictions to observational strategies pursued by teams at European Southern Observatory and instrumentation consortia at National Radio Astronomy Observatory.
He has received recognitions including fellowships and prizes awarded by organizations such as American Physical Society, Simons Foundation, and honors associated with societies including American Association for the Advancement of Science. His election to fellowship and invited lectureships placed him alongside recipients from institutions like Harvard University, Princeton University, and Caltech. He has been an invited speaker at conferences organized by International Astronomical Union, American Astronomical Society, and workshops at CERN and Perimeter Institute for Theoretical Physics. Grants and awards from agencies such as National Science Foundation and Department of Energy supported collaborations with groups at Brookhaven National Laboratory and Lawrence Livermore National Laboratory.
- "Cosmic microwave background polarization and primordial gravitational waves" — a paper cited by researchers at BICEP2, Planck Collaboration, and WMAP teams; influential across authors from Princeton University and Stanford University. - "Particle physics models for dark matter and detection strategies" — referenced in experimental proposals involving LUX-ZEPLIN, XENON1T, and Large Hadron Collider collaborations such as ATLAS and CMS. - Review articles on non-Gaussianity and inflationary constraints used by analysts at Atacama Cosmology Telescope and South Pole Telescope. - Contributions to edited volumes circulated among researchers at Institute for Advanced Study and Perimeter Institute for Theoretical Physics. (Select publications appear in journals read widely by members of American Physical Society and Institute of Physics communities.)
He resides near research hubs associated with California Institute of Technology and engages in outreach connected to public science initiatives at institutions such as NASA and Smithsonian Institution. Outside academia he has collaborations and interactions with scholars from Johns Hopkins University, Columbia University, and international partners at University of Tokyo and Université Paris-Saclay.
Category:American physicists Category:Theoretical cosmologists