The VERITAS gamma ray experiment is
currently my primary research interest.
Very High Energy Gamma Ray physics combines many of the scientific
interests of astrophysics and particle physics. For the particle
physicist, the cosmos contains the highest energy accelerators
available, and may ultimately prove to be the final frontier in
fundamental physics.
To date, very high-energy gamma rays have been observed from a variety
of sources (active galactic nuclei, pulsar-powered nebulae, supernova
remnants and an X-ray binary system), offering a wealth of scientific
information. Because gamma rays are not as strongly attenuated in the
galaxy as longer wavelength radiation, they offer a clear and unique
view through the galactic plane. In addition, because of their
interaction in infrared photon fields and in strong magnetic fields
via pair production, they can be used to probe
intergalactic
radiation fields. Finally, the highest energy gamma rays, which are
beyond any energies that can be produced on Earth, provide a unique
probe of many fundamental particle theories.
Much of the science of VHE gamma rays can be grouped into one of two
categories. The first concentrates on understanding the mechanism of
gamma ray production in cosmic sources and looking for new sources of
gamma rays. The second focuses on fundamental particle physics issues
that can be probed by nature's cosmic accelerators. Two studies in the
latter category have especially captured my interest at UMass:
measurement of gamma ray speeds (relevant to theories of Quantum
Gravity) and search for neutralino annhilation into gamma rays (an
important search for dark matter).
More details of UMass involvement in VERITAS can be found
here.