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Céline Bœhm

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Céline Bœhm
FInstP
Born1974 (age 49–50)[1]
Alma materÉcole normale supérieure
Pierre and Marie Curie University
École Polytechnique
Scientific career
FieldsDark matter
InstitutionsUniversity of Sydney
Durham University
University of Oxford
Perimeter Institute
Paris Observatory
Websitewww.ippp.dur.ac.uk/profile/cboehm

Céline Bœhm FInstP is a Professor of Particle Physics at the University of Sydney. She works on astroparticle physics and dark matter.

Early life and education

Bœhm studied fundamental physics at the Pierre and Marie Curie University, graduating in 1997.[2] She joined École Polytechnique, where she obtained a Master in Engineering in 1998.[2] She earned the highest distinction for a postgraduate diploma in theoretical physics.[2] She completed her PhD at the École normale supérieure in Paris in 2001, working with Pierre Fayet.[citation needed] She worked on supersymmetry, in the 4-body decay of the stop particle. She studied light scalar top quark and supersymmetric dark matter [3] She looked at collisional damping, which considers the impact of dark matter and standard model particles with the cosmic microwave background.[4]

Career and research

In 2001 Bœhm joined Joseph Silk at the University of Oxford. Here she worked on light dark matter particles which couple to light Z′ bosons.[5] She proposed new candidates for scalar dark matter, in the form of heavy fermions or light gauge bosons.[6] When the SPI spectrometer onboard INTEGRAL identified a 511 keV line in the Galactic Center, Bœhm predicted that this could have been the signature of dark matter.[7] She has continued to search for new signatures of dark matter, including examining the GeV excess in the Fermi Gamma-ray Space Telescope data.[8][9][10] In 2004 Bœhm joined the Laboratoire d'Annecy-le-Vieux de Physique Théorique, where she was promoted to senior lecturer in 2008.[11] She was awarded the Centre national de la recherche scientifique Bronze Medal.[11]

She looked at the analysis of the CoGeNT direct detection method, and found that it could have suffered from a large background.[12] In 2015 Boehm was nominated as Fellow of the Institute of Physics. She is the Principal investigator of the Theia mission, a space observatory which will allow Bœhm and her team to test the dark matter predictions that arise due to the Lambda-CDM model.[13][14]

Boehm was made an Emmy Noether Fellow at the Perimeter Institute for Theoretical Physics in 2016, where she continued to work on dark matter.[15][16] That year, she was promoted to Professor in the Institute for Particle Physics Phenomenology at Durham University. She gave a TED talk, The Invisible is All What Matters, at Durham in 2017.[17] Alongside her work in astroparticle physics, she works on non-crystallographic Coxeter groups.[18][19] She led the dark matter working package of the Euclid Consortium. In 2017 Bœhm spent two months as a visiting professor at Columbia University, as well as working at the Paris Observatory. She proposed using circular polarisation to study dark matter and neutrinos.[20] She joined the University of Sydney as Head of School for physics in 2018.[21][2] Bœhm has written for The Conversation.[22] She has taken part in Pint of Science.[23]

References

  1. ^ VIAF 197788028
  2. ^ a b c d "News | The University of Sydney". sydney.edu.au. Retrieved 2018-09-28.
  3. ^ Boehm, C.; Djouadi, A.; Drees, M. (2000-07-12). "Light Scalar Top Quarks and Supersymmetric Dark Matter". Physical Review D. 62 (3): 035012. arXiv:hep-ph/9911496. Bibcode:2000PhRvD..62c5012B. doi:10.1103/PhysRevD.62.035012. ISSN 0556-2821. S2CID 15138751.
  4. ^ "Celine Boehm | Institute for Particle Physics Phenomenology". www.ippp.dur.ac.uk. Archived from the original on 2019-04-01. Retrieved 2018-09-28.
  5. ^ Boehm, C.; Ensslin, T. A.; Silk, J. (2004-03-01). "Can annihilating Dark Matter be lighter than a few GeVs?". Journal of Physics G: Nuclear and Particle Physics. 30 (3): 279–285. arXiv:astro-ph/0208458. Bibcode:2004JPhG...30..279B. doi:10.1088/0954-3899/30/3/004. ISSN 0954-3899. S2CID 119056668.
  6. ^ Boehm, C.; Fayet, P. (2004). "Scalar Dark Matter candidates". Nuclear Physics B. 683 (1–2): 219–263. arXiv:hep-ph/0305261. Bibcode:2004NuPhB.683..219B. doi:10.1016/j.nuclphysb.2004.01.015. S2CID 17516917.
  7. ^ Boehm, Celine; Hooper, Dan; Silk, Joseph; Casse, Michel (2004-03-12). "MeV Dark Matter: Has It Been Detected?". Physical Review Letters. 92 (10): 101301. arXiv:astro-ph/0309686. Bibcode:2004PhRvL..92j1301B. doi:10.1103/PhysRevLett.92.101301. ISSN 0031-9007. PMID 15089189. S2CID 17988955.
  8. ^ Boehm, Celine; Dolan, Matthew J.; McCabe, Christopher; Spannowsky, Michael; Wallace, Chris J. (2014-05-08). "Extended gamma-ray emission from Coy Dark Matter". Journal of Cosmology and Astroparticle Physics. 2014 (5): 009. arXiv:1401.6458. Bibcode:2014JCAP...05..009B. doi:10.1088/1475-7516/2014/05/009. ISSN 1475-7516. S2CID 119184166.
  9. ^ Lacroix, Thomas; Boehm, Celine; Silk, Joseph (2014-08-08). "Fitting the Fermi-LAT GeV excess: On the importance of including the propagation of electrons from dark matter". Physical Review D. 90 (4): 043508. arXiv:1403.1987. Bibcode:2014PhRvD..90d3508L. doi:10.1103/PhysRevD.90.043508. ISSN 1550-7998. S2CID 55698259.
  10. ^ Boehm, Celine; Dolan, Matthew J.; McCabe, Christopher (2014-07-22). "A weighty interpretation of the Galactic Centre excess". Physical Review D. 90 (2): 023531. arXiv:1404.4977. doi:10.1103/PhysRevD.90.023531. ISSN 1550-7998.
  11. ^ a b "celineboehm@lapth". sites.google.com. Retrieved 2018-09-28.[permanent dead link‍]
  12. ^ Davis, Jonathan H.; McCabe, Christopher; Boehm, Celine (2014-08-06). "Quantifying the evidence for Dark Matter in CoGeNT data". Journal of Cosmology and Astroparticle Physics. 2014 (8): 014. arXiv:1405.0495. Bibcode:2014JCAP...08..014D. doi:10.1088/1475-7516/2014/08/014. ISSN 1475-7516. S2CID 54532870.
  13. ^ The Theia Collaboration; Boehm, Celine; Krone-Martins, Alberto; Amorim, Antonio; Anglada-Escude, Guillem; Brandeker, Alexis; Courbin, Frederic; Ensslin, Torsten; Falcao, Antonio (2017-07-02). "Theia: Faint objects in motion or the new astrometry frontier". arXiv:1707.01348. {{cite journal}}: Cite journal requires |journal= (help)
  14. ^ "Theia meeting | Institute for Particle Physics Phenomenology". www.ippp.dur.ac.uk. Archived from the original on 2018-09-29. Retrieved 2018-09-28.
  15. ^ "Celine Boehm | Perimeter Institute". www.perimeterinstitute.ca. Retrieved 2018-09-28.
  16. ^ Wonders of Physics (2016-05-09), Dark Matter with Dr Celine Boehm, retrieved 2018-09-28
  17. ^ TEDx Talks (2017-01-26), The Invisible is All What Matters | Dr. Celine Boehm | TEDxDurhamUniversity, retrieved 2018-09-28
  18. ^ Dechant, Pierre-Philippe; Boehm, Celine; Twarock, Reidun (2013). "Affine extensions of non-crystallographic Coxeter groups induced by projection". Journal of Mathematical Physics. 54 (9): 093508. arXiv:1110.5228. Bibcode:2013JMP....54i3508D. doi:10.1063/1.4820441. ISSN 0022-2488. S2CID 59469917.
  19. ^ Dechant, Pierre-Philippe; Boehm, Celine; Twarock, Reidun (2012-07-20). "Novel Kac-Moody-type affine extensions of non-crystallographic Coxeter groups". Journal of Physics A: Mathematical and Theoretical. 45 (28): 285202. arXiv:1110.5219. Bibcode:2012JPhA...45B5202D. doi:10.1088/1751-8113/45/28/285202. ISSN 1751-8113. S2CID 44541666.
  20. ^ Bœhm, Céline; Degrande, Céline; Mattelaer, Olivier; Vincent, Aaron C. (2017). "Circular polarisation: a new probe of dark matter and neutrinos in the sky". Journal of Cosmology and Astroparticle Physics. 2017 (5): 043. arXiv:1701.02754. Bibcode:2017JCAP...05..043B. doi:10.1088/1475-7516/2017/05/043. ISSN 1475-7516. S2CID 54747614.
  21. ^ "Subscribe to The Australian | Newspaper home delivery, website, iPad, iPhone & Android apps". www.theaustralian.com.au. Retrieved 2018-09-28.
  22. ^ "Celine Boehm". The Conversation. Retrieved 2018-09-28.
  23. ^ "Science on the Grand Scale". Pint of Science. Retrieved 2018-09-28.
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