Graciela Gelmini Explained

Graciela Gelmini
Birth Name:Graciela Beatriz Gelmini
Birth Place:Argentina
Fields:Particle physics
Workplaces:Ludwig Maximilian University of Munich
ICTP (1982 – 1989)
UCLA (1989 – present)
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Thesis Year:1981
Doctoral Advisor:Roberto Peccei
Carlos A. Garcia Canal
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Graciela Beatriz Gelmini is a theoretical physicist who specializes in astroparticle physics.[1] [2] She is a professor at the University of California, Los Angeles (UCLA),[3] and became a fellow of the American Physical Society in 2004.[4]

Early life and career

Gelmini received her Ph.D. from the National University of La Plata in 1981.[5] Her doctoral advisors were Roberto Peccei and Carlos A. Garcia Canal.

Upon graduation, Gelmini worked at the Ludwig Maximilian University of Munich in Germany for a few years before moving to the International Centre for Theoretical Physics in Italy at around 1982.[6] [7] During this time, she was based at CERN in Switzerland.[8] [9] Gelmini was also affiliated with the Lyman Laboratory of Physics at Harvard University and the Enrico Fermi Institute at the University of Chicago between 1986 and 1988.[10] [11]

In November 1989, Gelmini joined UCLA as a faculty member and has been there ever since.[12]

Scientific contributions

In November 2007, Gelmini was part of a team that analyzed data from the Pierre Auger Observatory in Argentina and discovered high-energy particles that made it to Earth from nearby black holes.[13] [14]

Publications

Notes and References

  1. Gondolo. Paolo. Gelmini. Graciela. 1991. Cosmic abundances of stable particles: Improved analysis. Nuclear Physics B. en. 360. 1. 145–179. 10.1016/0550-3213(91)90438-4. 1991NuPhB.360..145G. 0550-3213.
  2. Gelmini. Graciela. Gondolo. Paolo. 2006. Neutralino with the right cold dark matter abundance in (almost) any supersymmetric model. Physical Review D. 74. 2. 023510. 10.1103/PhysRevD.74.023510. hep-ph/0602230. 2006PhRvD..74b3510G. 37865240.
  3. Web site: Graciela Gelmini. 2021-04-15. UCLA Physics & Astronomy.
  4. Web site: APS Fellow Archive. 2021-04-15. American Physical Society. en.
  5. Web site: INSPIRE-HEP Graciela B. Gelmini. 2021-04-15. inspirehep.net.
  6. Gelmini. Graciela B.. Nussinov. Shmuel. Roncadelli. Marco. 1982. Bounds and prospects for the majoron model of left-handed neutrino masses. Nuclear Physics B. en. 209. 1. 157–173. 10.1016/0550-3213(82)90107-9. 1982NuPhB.209..157G . 0550-3213.
  7. Baldeschi. M. R.. Gelmini. G. B.. Ruffini. R.. 1983. On massive fermions and bosons in galactic halos. Physics Letters B. en. 122. 3–4. 221–224. 10.1016/0370-2693(83)90688-3. 1983PhLB..122..221B . 0370-2693.
  8. Gelmini. G. B.. Nanopoulos. D. V.. Olive. K. A.. 1983. Finite temperature effects in primordial inflation. Physics Letters B. en. 131. 1–3. 53–58. 10.1016/0370-2693(83)91090-0. 1983PhLB..131...53G . 0370-2693.
  9. Buccella. Franco. Gelmini. Graciela B.. Masiero. Antonio. Roncadelli. Marco. 1984. The Majoron and left-handed neutrino masses in SU(5). Nuclear Physics B. en. 231. 3. 493–505. 10.1016/0550-3213(84)90516-9. 1984NuPhB.231..493B . 0550-3213.
  10. Gelmini. G. B.. Hall. L. J.. Lin. M. J.. 1987. What is the cosmion?. Nuclear Physics B. en. 281. 3–4. 726–735. 10.1016/0550-3213(87)90424-X. 1987NuPhB.281..726G . 0550-3213.
  11. Gelmini. G.. 1986. Bounds on galactic cold dark matter particle candidates and solar axions from a Ge-spectrometer. 6739649. English. osti.gov.
  12. Gelmini. Graciela B.. Gondolo. P.. Roulet. E.. 1991. Neutralino dark matter searches. Nuclear Physics B. en. 351. 3. 623–644. 10.1016/S0550-3213(05)80036-7. 1991NuPhB.351..623G . 0550-3213.
  13. Web site: Wolpert. Stuart. 2007-11-09. High-energy particles from violent black holes travel to Earth. 2021-04-15. EurekAlert!. en.
  14. The Pierre Auger Collaboration. 2007. Correlation of the Highest-Energy Cosmic Rays with Nearby Extragalactic Objects. Science. en. 318. 5852. 938–943. 10.1126/science.1151124. 0036-8075. 17991855. 0711.2256. 2007Sci...318..938P. 118376969 .