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Edsjo thesis

These interaction rates and cross sections are generally computed with standard, one- or two-parameter model-dependent nuclear form factors, which may not exactly mirror the actual form factor for the particular nucleus in question. With neutrino masses and dark matter being two of only a handful of indications for BSM physics and new generations of experiments just around the corner, these fields are likely to remain fruitful for many years to come and receive attention from the physics community. My research interests are focused on phenomenology of neutrino physics, beyond the standard model (BSM) physics, dark matter, and extra dimensions.

Edsjo thesis

Edsjo thesis

(talk in pdf) SUSY Dark Matter: Loops and Precision from Particle Physics invited talk at RADCOR05, Sokendai, Japan, October 2005. Theoretical calculations of neutralino–nucleon interaction rates with various nuclei are of great interest to direct dark matter searches such as CDMS, EDELWEISS, ZEPLIN and other experiments since they are used to establish upper bounds on the WIMP–proton cross section.

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  • Furthermore, I am continuously trying to broaden my research into nearby fields.


    Edsjo thesis

    Edsjo thesis

    Edsjo thesis

    As is well known, elastic electron scattering can allow for very precise determinations of nuclear form factors and hence nuclear charge densities for spherical or near-spherical nuclei. Galaxy and dark-matter halo evolution in different cosmologies.

    Edsjo thesis

    Edsjö received his Ph D in 1997 from the Uppsala University, with a thesis by the title of "Aspects of neutrino detection of neutralino dark matter". OXFORD BOOK OF ESSAY I have also been involved in training courses for teachers and have given a lot of popular science lectures.


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