Department of Physics

Staff profile

Dr Celine Boehm

Lecturer in the Department of Physics

Contact Dr Celine Boehm (email at c.m.boehm@durham.ac.uk)

Research Groups

  • Elementary Particle Theory

Publications

  • 1: Albornoz-Vasquez, Daniel Belanger, Genevieve Boehm, Celine , Pukhov, Alexander & Silk, Joseph (2010). Can neutralinos in the MSSM and NMSSM scenarios still be light?. Physical Review D 82(11): 115027
  • 2: Boehm, Celine , Delahaye, Timur & Silk, Joseph (2010). Can the morphology of gamma-ray emission distinguish annihilating from decaying dark matter?. Physical Review Letters 105(22): 221301.
  • 3: Boehm, Celine , Silk, Joseph & Ensslin, Torsten (2012). Radio observations of the Galactic Centre and the Coma cluster as a probe of light dark matter self-annihilations and decay.
  • 4: Albornoz Vásquez, Daniel, Bélanger, Geneviève & Boehm, Céline (2011). Astrophysical limits on light NMSSM neutralinos. Physical Review D 84(9): 095008.
  • Dechant, P.-P., Boehm, C. & Twarock, R. (2011). Affine extensions of non-crystallographic Coxeter groups induced by projection. ArXiv e-prints
  • Delahaye, Timur, Boehm, Celine & Silk, Joseph (2011). Can Planck constrain indirect detection of dark matter in our galaxy? Monthly Notices of the Royal Astronomy Society
  • Albornoz Vasquez, Daniel, Belanger, Genevieve & Boehm, Celine (2011). Revisiting light neutralino scenarios in the MSSM. Physical Review D84: 095015.
  • Vasquez, Daniel Albornoz, Boehm, Celine & Idarraga, John (2011). Signature of Sub GeV Dark Matter particles at LHC and TEVATRON. Physical Review D83: 115017.
  • Boehm, Celine, Delahaye, Timur, Salati, Pierre, Staub, Florian & Singh, Ritesh K. (2010). Implication of the PAMELA antiproton data for dark matter indirect detection at LHC. Journal of Cosmology and Astroparticle Physics 1006: 013.
  • Lavalle, Julien, Boehm, Celine & Barthes, Julien (2010). On the Sunyaev-Zel'dovich effect from dark matter annihilation or decay in galaxy clusters. Journal of Cosmology and Astroparticle Physics 1002: 005.
  • Prantzos, N., Boehm, C., Bykov, A.M., Diehl, R., Ferriere, K. & others (2010). The 511 keV emission from positron annihilation in the Galaxy.
  • Boehm, Celine & Lavalle, Julien (2009). Clarifying the covariant formalism for the SZ effect due to relativistic non-thermal electrons. Physical Review D79: 083505.
  • Boehm, Celine & Silk, Joseph (2008). A New test of the light dark matter hypothesis. Physics Letters B661: 287-289.
  • Boehm, Celine, Farzan, Yasaman, Hambye, Thomas, Palomares-Ruiz, Sergio & Pascoli, Silvia (2008). Is it possible to explain neutrino masses with scalar dark matter? Physical Review D77: 043516.
  • Boehm, Celine (2008). Thirty years of research in cosmology, particle physics and astrophysics and how many more to discover dark matter? Review of Modern Astronomy 20: 107-139.
  • Boehm, C. (2007). Will the discovery of the nature of dark matter match expectations? 17-29.
  • Ascasibar, Yago, Jean, P., Boehm, C. & Knoedlseder, J. (2006). Constraints on dark matter and the shape of the Milky Way dark halo from the 511-keV line. Monthly Notices of the Royal Astronomy Society 368: 1695-1705.
  • Skordis, Constantinos, Mota, D.F., Ferreira, P.G. & Boehm, C. (2006). Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics. Physical Review Letters 96: 011301.
  • Boehm, C., Orloff, J. & Salati, P. (2006). Light Dark Matter Annihilations into Two Photons. Physics Letters B641: 247-253.
  • Boehm, C. & Uwer, P. (2006). Revisiting Bremsstrahlung emission associated with Light Dark Matter annihilations.
  • Boehm, C., Ensslin, T.A. & Silk, J. (2004). Can Annihilating dark matter be lighter than a few GeVs? Journal of Physics G G30: 279-286.
  • Boehm, Celine & Schaeffer, Richard (2004). Constraints on dark matter interactions from structure formation: Damping lengths. Astronomy and Astrophysics
  • Boehm, Celine (2004). Implications of a new light gauge boson for neutrino physics. Physical Review D70: 055007.
  • Boehm, C., Fayet, Pierre & Silk, J. (2004). Light and heavy dark matter particles. Physical Review D69: 101302.
  • Boehm, Celine, Hooper, Dan, Silk, Joseph, Casse, Michel & Paul, Jacques (2004). MeV dark matter: Has it been detected? Physical Review Letters 92: 101301.
  • Boehm, Celine & Ascasibar, Yago (2004). More evidence in favour of light dark matter particles? Physical Review D70: 115013.
  • Hooper, Dan, Ferrer, Francesc, Boehm, Celine, Silk, Joseph, Paul, Jacques & others (2004). Possible evidence for MeV dark matter in dwarf spheroidals. Physical Review Letters 93: 161302.
  • Boehm, C. & Fayet, Pierre (2004). Scalar dark matter candidates. Nuclear Physics B683: 219-263.
  • Boehm, C. (2004). Structure formation for light annihilating dark matter. Int.J.Mod.Phys A19: 4355-4365.
  • Boehm, C. (2003). A light dark matter signature? AHEP2003/065.
  • Boehm, C., Mathis, H., Devriendt, J. & Silk, J. (2003). WIMP matter power spectra and small scale power generation. Monthly Notices of the Royal Astronomy Society
  • Boehm, Celine, Fayet, Pierre & Schaeffer, Richard (2002). Constraining the strength of dark matter interactions from structure formation. 333-344.
  • Boehm, C. (2002). Dark matter photon interactions: Are they allowed? 345-355.
  • Boehm, Celine, Riazuelo, Alain, Hansen, Steen H. & Schaeffer, Richard (2002). Interacting dark matter disguised as warm dark matter. Physical Review D66: 083505.
  • Boehm, C., Fayet, Pierre & Schaeffer, R. (2001). Constraining dark matter candidates from structure formation. Physics Letters B518: 8-14.
  • Boehm, C., Djouadi, A. & Mambrini, Y. (2000). Decays of the lightest top squark. Physical Review D61: 095006.
  • Boehm, Celine, Djouadi, Abdelhak & Drees, Manuel (2000). Light scalar top quarks and supersymmetric dark matter. Physical Review D62: 035012.
  • Gangui, Alejandro, Peter, Patrick & Boehm, Celine (1998). Could electromagnetic corrections solve the vorton excess problem? Physical Review D57: 2580-2589.
  • Djouadi, A. & others (1998). The Minimal supersymmetric standard model: Group summary report.

Supervises