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Madappa Prakash

Madappa Prakash (born December 28, 1953, in Mysore) is an Indian-American nuclear physicist and astrophysicist, known for his research on the physics of neutron stars and heavy-ion collisions.[1]

Education and career edit

Prakash grew up in Mysore. At the University of Mysore he graduated with a bachelor's degree in 1971 and a master's degree in 1973. At the University of Bombay (now the University of Mumbai), he received his PhD in 1979 with a dissertation on nuclear fission. From 1974 to 1981, he held a position as a scientific officer at the Bhabha Atomic Research Centre. As a postdoc, he was from 1979 to 1981 on leave of absence for study and research at Copenhagen's Niels Bohr Institute. At the State University of New York at Stony Brook he taught and did research from 1982 to 2005 and collaborated extensively with James Lattimer. From 2005 to the present, Prakash is a professor at Ohio University.[2] In 2020 he and another Ohio University professor became participants in the Network for Neutrinos, Nuclear Astrophysics, and Symmetries (N3AS) Physics Frontier Center, with headquarters at the University of California, Berkeley.[3][4]

Prakash's research deals with neutron stars and with atomic nuclei and nuclear matter under extreme conditions of density, temperature, and magnetic fields.[2][5] In 2022, he won the Hans A. Bethe Prize, the most prestigious prize in the field of nuclear astrophysics, for his research about neutron stars and black holes.

Investigations of strangeness-bearing matter led him to discover new pathways to form stellar mass black holes from metastable neutron stars. His work includes the evolution of neutron stars from their birth to old age, neutrino interactions and propagation in dense astrophysical systems, and the theoretical interpretations of the growing number of observations of neutron stars. He develops equations of state, neutrino opacities, and transport characteristics in dense matter for studies of supernovae and binary mergers involving neutron stars and black holes.[2]

In 2001 Prakash was elected a Fellow of the American Physical Society for "fundamental research into the properties of hot and dense matter, providing a basis for understanding relativistic heavy ion collisions and the structure and composition of neutron stars."[6] In 2022 he received the Hans A. Bethe Prize with citation:

For fundamental contributions to the physics of hot and dense matter, and their implications for heavy ion collisions and multi-messenger observations of neutron star structure and evolution.[5]

Selected publications edit

  • Müther, H.; Prakash, M.; Ainsworth, T.L. (1987). "The nuclear symmetry energy in relativistic Brueckner-Hartree-Fock calculations". Physics Letters B. 199 (4): 469–474. Bibcode:1987PhLB..199..469M. doi:10.1016/0370-2693(87)91611-X.
  • Prakash, M.; Ainsworth, T. L.; Lattimer, J. M. (1988). "Equation of State and the Maximum Mass of Neutron Stars". Physical Review Letters. 61 (22): 2518–2521. Bibcode:1988PhRvL..61.2518P. doi:10.1103/PhysRevLett.61.2518. PMID 10039146.
  • Lattimer, James M.; Pethick, C. J.; Prakash, Madappa; Haensel, Pawel (1991). "Direct URCA process in neutron stars". Physical Review Letters. 66 (21): 2701–2704. Bibcode:1991PhRvL..66.2701L. doi:10.1103/PhysRevLett.66.2701. PMID 10043594. (over 850 citations)
  • Prakash, M. (1997). "Composition and structure of protoneutron stars". Physics Reports. 280: 1–77. arXiv:nucl-th/9603042. Bibcode:1997PhR...280....1P. doi:10.1016/S0370-1573(96)00023-3. S2CID 1770109.
  • Pons, J. A.; Reddy, S.; Prakash, M.; Lattimer, J. M.; Miralles, J. A. (1999). "Evolution of Proto–Neutron Stars". The Astrophysical Journal. 513 (2): 780–804. arXiv:astro-ph/9807040. Bibcode:1999ApJ...513..780P. doi:10.1086/306889. S2CID 10501821.
  • Lattimer, J. M.; Prakash, M. (2001). "Neutron Star Structure and the Equation of State". The Astrophysical Journal. 550 (1): 426–442. arXiv:astro-ph/0002232. Bibcode:2001ApJ...550..426L. doi:10.1086/319702. S2CID 14782250. (over 1700 citations)
  • Lattimer, J. M.; Prakash, M. (2004). "The Physics of Neutron Stars". Science. 304 (5670): 536–542. arXiv:astro-ph/0405262. Bibcode:2004Sci...304..536L. doi:10.1126/science.1090720. PMID 15105490. S2CID 10769030. (over 1500 citations)
  • Page, Dany; Lattimer, James M.; Prakash, Madappa; Steiner, Andrew W. (2004). "Minimal Cooling of Neutron Stars: A New Paradigm". The Astrophysical Journal Supplement Series. 155 (2): 623–650. arXiv:astro-ph/0403657. Bibcode:2004ApJS..155..623P. doi:10.1086/424844. S2CID 2141379.
  • Steiner, A.W.; Prakash, M.; Lattimer, J.M.; Ellis, P.J. (2005). "Isospin asymmetry in nuclei and neutron stars". Physics Reports. 411 (6): 325–375. arXiv:nucl-th/0410066. doi:10.1016/j.physrep.2005.02.004. S2CID 119087712. (over 1000 citations)
  • Lattimer, J.; Prakash, M. (2007). "Neutron star observations: Prognosis for equation of state constraints". Physics Reports. 442 (1–6): 109–165. arXiv:astro-ph/0612440. Bibcode:2007PhR...442..109L. doi:10.1016/j.physrep.2007.02.003. S2CID 53523635. (over 1550 citations)
  • Page, Dany; Prakash, Madappa; Lattimer, James M.; Steiner, Andrew W. (2011). "Rapid Cooling of the Neutron Star in Cassiopeia a Triggered by Neutron Superfluidity in Dense Matter". Physical Review Letters. 106 (8): 081101. arXiv:1011.6142. Bibcode:2011PhRvL.106h1101P. doi:10.1103/PhysRevLett.106.081101. PMID 21405561. S2CID 423395.
  • Lattimer, James M.; Prakash, Madappa (2016). "The equation of state of hot, dense matter and neutron stars". Physics Reports. 621: 127–164. arXiv:1512.07820. Bibcode:2016PhR...621..127L. doi:10.1016/j.physrep.2015.12.005. S2CID 118514019.
  • Prakash, Madappa (2014). "Neutron stars as probes of extreme energy density matter". Pramana. 84 (5): 927. arXiv:1404.1966. Bibcode:2015Prama..84..927P. doi:10.1007/s12043-015-0979-7. S2CID 118472033.
  • Drischler, Christian; Han, Sophia; Lattimer, James M.; Prakash, Madappa; Reddy, Sanjay; Zhao, Tianqi (2021). "Limiting masses and radii of neutron stars and their implications". Physical Review C. 103 (4): 045808. arXiv:2009.06441. Bibcode:2021PhRvC.103d5808D. doi:10.1103/PhysRevC.103.045808. S2CID 221655657.

References edit

  1. ^ "Madappa Prakash awarded most prestigious prize in nuclear astrophysics". College of Arts & Sciences Forum, Ohio University. October 20, 2021.
  2. ^ a b c "Madappa Prakash, Bio". Physics & Astronomy Department, Ohio University.
  3. ^ "Prakash, Phillips Part of New Physics Frontier Center on Neutron Star Modeling". College of Arts & Sciences Forum, Ohio University. August 18, 2020.
  4. ^ "UC Berkeley Center Will Model Neutron Star Mergers". News Center, Berkeley Lab. August 17, 2020.
  5. ^ a b "2022 Hans A. Bethe Prize Recipient, Madappa Prakash". American Physical Society.
  6. ^ "APS Fellow Archive". American Physical Society. (search on year=2001 and institution=SUNY at Stony Brook)

madappa, prakash, born, december, 1953, mysore, indian, american, nuclear, physicist, astrophysicist, known, research, physics, neutron, stars, heavy, collisions, education, career, editprakash, grew, mysore, university, mysore, graduated, with, bachelor, degr. Madappa Prakash born December 28 1953 in Mysore is an Indian American nuclear physicist and astrophysicist known for his research on the physics of neutron stars and heavy ion collisions 1 Education and career editPrakash grew up in Mysore At the University of Mysore he graduated with a bachelor s degree in 1971 and a master s degree in 1973 At the University of Bombay now the University of Mumbai he received his PhD in 1979 with a dissertation on nuclear fission From 1974 to 1981 he held a position as a scientific officer at the Bhabha Atomic Research Centre As a postdoc he was from 1979 to 1981 on leave of absence for study and research at Copenhagen s Niels Bohr Institute At the State University of New York at Stony Brook he taught and did research from 1982 to 2005 and collaborated extensively with James Lattimer From 2005 to the present Prakash is a professor at Ohio University 2 In 2020 he and another Ohio University professor became participants in the Network for Neutrinos Nuclear Astrophysics and Symmetries N3AS Physics Frontier Center with headquarters at the University of California Berkeley 3 4 Prakash s research deals with neutron stars and with atomic nuclei and nuclear matter under extreme conditions of density temperature and magnetic fields 2 5 In 2022 he won the Hans A Bethe Prize the most prestigious prize in the field of nuclear astrophysics for his research about neutron stars and black holes Investigations of strangeness bearing matter led him to discover new pathways to form stellar mass black holes from metastable neutron stars His work includes the evolution of neutron stars from their birth to old age neutrino interactions and propagation in dense astrophysical systems and the theoretical interpretations of the growing number of observations of neutron stars He develops equations of state neutrino opacities and transport characteristics in dense matter for studies of supernovae and binary mergers involving neutron stars and black holes 2 In 2001 Prakash was elected a Fellow of the American Physical Society for fundamental research into the properties of hot and dense matter providing a basis for understanding relativistic heavy ion collisions and the structure and composition of neutron stars 6 In 2022 he received the Hans A Bethe Prize with citation For fundamental contributions to the physics of hot and dense matter and their implications for heavy ion collisions and multi messenger observations of neutron star structure and evolution 5 Selected publications editThis section may contain excessive or irrelevant examples Please help improve the article by adding descriptive text and removing less pertinent examples July 2023 Muther H Prakash M Ainsworth T L 1987 The nuclear symmetry energy in relativistic Brueckner Hartree Fock calculations Physics Letters B 199 4 469 474 Bibcode 1987PhLB 199 469M doi 10 1016 0370 2693 87 91611 X Prakash M Ainsworth T L Lattimer J M 1988 Equation of State and the Maximum Mass of Neutron Stars Physical Review Letters 61 22 2518 2521 Bibcode 1988PhRvL 61 2518P doi 10 1103 PhysRevLett 61 2518 PMID 10039146 Lattimer James M Pethick C J Prakash Madappa Haensel Pawel 1991 Direct URCA process in neutron stars Physical Review Letters 66 21 2701 2704 Bibcode 1991PhRvL 66 2701L doi 10 1103 PhysRevLett 66 2701 PMID 10043594 over 850 citations Prakash M 1997 Composition and structure of protoneutron stars Physics Reports 280 1 77 arXiv nucl th 9603042 Bibcode 1997PhR 280 1P doi 10 1016 S0370 1573 96 00023 3 S2CID 1770109 Pons J A Reddy S Prakash M Lattimer J M Miralles J A 1999 Evolution of Proto Neutron Stars The Astrophysical Journal 513 2 780 804 arXiv astro ph 9807040 Bibcode 1999ApJ 513 780P doi 10 1086 306889 S2CID 10501821 Lattimer J M Prakash M 2001 Neutron Star Structure and the Equation of State The Astrophysical Journal 550 1 426 442 arXiv astro ph 0002232 Bibcode 2001ApJ 550 426L doi 10 1086 319702 S2CID 14782250 over 1700 citations Lattimer J M Prakash M 2004 The Physics of Neutron Stars Science 304 5670 536 542 arXiv astro ph 0405262 Bibcode 2004Sci 304 536L doi 10 1126 science 1090720 PMID 15105490 S2CID 10769030 over 1500 citations Page Dany Lattimer James M Prakash Madappa Steiner Andrew W 2004 Minimal Cooling of Neutron Stars A New Paradigm The Astrophysical Journal Supplement Series 155 2 623 650 arXiv astro ph 0403657 Bibcode 2004ApJS 155 623P doi 10 1086 424844 S2CID 2141379 Steiner A W Prakash M Lattimer J M Ellis P J 2005 Isospin asymmetry in nuclei and neutron stars Physics Reports 411 6 325 375 arXiv nucl th 0410066 doi 10 1016 j physrep 2005 02 004 S2CID 119087712 over 1000 citations Lattimer J Prakash M 2007 Neutron star observations Prognosis for equation of state constraints Physics Reports 442 1 6 109 165 arXiv astro ph 0612440 Bibcode 2007PhR 442 109L doi 10 1016 j physrep 2007 02 003 S2CID 53523635 over 1550 citations Page Dany Prakash Madappa Lattimer James M Steiner Andrew W 2011 Rapid Cooling of the Neutron Star in Cassiopeia a Triggered by Neutron Superfluidity in Dense Matter Physical Review Letters 106 8 081101 arXiv 1011 6142 Bibcode 2011PhRvL 106h1101P doi 10 1103 PhysRevLett 106 081101 PMID 21405561 S2CID 423395 Lattimer James M Prakash Madappa 2016 The equation of state of hot dense matter and neutron stars Physics Reports 621 127 164 arXiv 1512 07820 Bibcode 2016PhR 621 127L doi 10 1016 j physrep 2015 12 005 S2CID 118514019 Prakash Madappa 2014 Neutron stars as probes of extreme energy density matter Pramana 84 5 927 arXiv 1404 1966 Bibcode 2015Prama 84 927P doi 10 1007 s12043 015 0979 7 S2CID 118472033 Drischler Christian Han Sophia Lattimer James M Prakash Madappa Reddy Sanjay Zhao Tianqi 2021 Limiting masses and radii of neutron stars and their implications Physical Review C 103 4 045808 arXiv 2009 06441 Bibcode 2021PhRvC 103d5808D doi 10 1103 PhysRevC 103 045808 S2CID 221655657 References edit Madappa Prakash awarded most prestigious prize in nuclear astrophysics College of Arts amp Sciences Forum Ohio University October 20 2021 a b c Madappa Prakash Bio Physics amp Astronomy Department Ohio University Prakash Phillips Part of New Physics Frontier Center on Neutron Star Modeling College of Arts amp Sciences Forum Ohio University August 18 2020 UC Berkeley Center Will Model Neutron Star Mergers News Center Berkeley Lab August 17 2020 a b 2022 Hans A Bethe Prize Recipient Madappa Prakash American Physical Society APS Fellow Archive American Physical Society search on year 2001 and institution SUNY at Stony Brook Retrieved from https en wikipedia org w index php title Madappa Prakash amp oldid 1182206610, wikipedia, wiki, book, books, library,

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