Michael Lester Norman
Affiliations: | 1986-2000 | Physics | University of Illinois, Urbana-Champaign, Urbana-Champaign, IL |
| 2000- | Physics | University of California, San Diego, La Jolla, CA |
Area:
Computational AstrophysicsWebsite:
https://physics.ucsd.edu/fac_staff/fac_profile/faculty_description.php?person_id=167Google:
"Michael Lester Norman"Bio:
http://www.sdsc.edu/about_sdsc/director.html
http://library.nd.edu/chemistry/resources/genealogy/physics/documents/NormanML.pdf
https://inspirehep.net/record/1028794?ln=en
Norman, M.L., Numerical study of rotating interstellar clouds: equilibrium and collapse California Univ., Livermore (USA). Lawrence Livermore Lab.
Mean distance: 14.01
Parents
Sign in to add mentor| James Ricker Wilson | grad student | 1980 | UC Davis | |
| (A numerical study of rotating interstellar clouds: equilibrium and collapse.) | ||||
Children
Sign in to add trainee| Dinshaw S. Balsara | grad student | 1990 | UIUC |
| Wen-Ching Lin | grad student | 2003 | UIUC |
| Brian W. O'Shea | grad student | 2005 | UIUC |
| Paschalis Paschos | grad student | 2005 | UIUC |
| Daniel J. Whalen | grad student | 2006 | UIUC |
| David C. Collins | grad student | 2009 | UCSD |
| Hao Xu | grad student | 2009 | UCSD |
| Stephen Skory | grad student | 2010 | UCSD |
| Geoffrey C. So | grad student | 2013 | UCSD |
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Publications
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| Regan JA, Wise JH, O’Shea BW, et al. (2020) The emergence of the first star-free atomic cooling haloes in the Universe Monthly Notices of the Royal Astronomical Society. 492: 3021-3031 |
| Wise JH, Regan JA, O'Shea BW, et al. (2019) Formation of massive black holes in rapidly growing pre-galactic gas clouds. Nature |
| Norman ML, Chen P, Wise JH, et al. (2018) Fully Coupled Simulation of Cosmic Reionization. III. Stochastic Early Reionization by the Smallest Galaxies The Astrophysical Journal. 867: 27 |
| Norman ML, Smith BD, Bordner J. (2018) Simulating the Cosmic Dawn With Enzo Frontiers in Astronomy and Space Sciences. 5: 34 |
| Smith BD, Regan JA, Downes TP, et al. (2018) The growth of black holes from Population III remnants in the Renaissance simulations Monthly Notices of the Royal Astronomical Society. 480: 3762-3773 |
| Barrow KSS, Wise JH, Aykutalp A, et al. (2017) First light – II. Emission line extinction, population III stars, and X-ray binaries Monthly Notices of the Royal Astronomical Society. 474: 2617-2634 |
| Barrow KSS, Wise JH, Norman ML, et al. (2017) First light: exploring the spectra of high-redshift galaxies in the Renaissance Simulations Monthly Notices of the Royal Astronomical Society. 469: 4863-4878 |
| Kritsuk A, Ustyugov S, Norman M. (2017) The structure and statistics of interstellar turbulence New Journal of Physics. 19: 65003 |
| Xu H, Ahn K, Norman ML, et al. (2016) X-RAY BACKGROUND AT HIGH REDSHIFTS FROM POP III REMNANTS: RESULTS FROM POP III STAR FORMATION RATES IN THE RENAISSANCE SIMULATIONS The Astrophysical Journal. 832: L5 |
| Xu H, Wise JH, Norman ML, et al. (2016) GALAXY PROPERTIES AND UV ESCAPE FRACTIONS DURING THE EPOCH OF REIONIZATION: RESULTS FROM THE RENAISSANCE SIMULATIONS The Astrophysical Journal. 833: 84 |