Faces in Research

Introduction
Physics Home
Physics Research Groups

Experimental Particle Physics
Dr. David Asner
Dr. Alain Bellerive
Dr. Madhu Dixit
Dr. Kevin Graham
Dr. Richard Hemingway
Dr. Gerald Oakham
Dr. David Sinclair
Dr. Manuella Vincter

Theoretical Particle Physics
Dr. Bruce Campbell
Dr. Steven Godfrey
Dr. Pat Kalyniak
Dr. Heather Logan
Dr. Peter Watson

Medical Physics
Dr. Boguslaw Jarosz
Dr. Paul Johns
Dr. David Rogers
Dr. Tong Xu

Photonics
Dr. John Armitage

Adjunct Professors
Dr. Ian Cameron
Dr. Brenda Clark
Dr. Joanna Cygler
Dr. Robert de Kemp
Dr. Lee Gerig
Dr. Cliff Hargrove
Dr. Iwan Kawrakow
Dr. Malcolm McEwen
Dr. Cheng Ng
Dr. Peter Raaphorst
Dr. Carl Ross
Dr. Richard Wassenar
Dr. R. Glenn Wells
Dr. David Wilkins
Dr. Ruth Wilkins

Dr. Kevin Graham
Assistant Professor of Physics
Ph.D. (Victoria)

Email: Kevin_Grahamphysics.carleton.ca

Involvement
SNOLab, EXO, DEAP

Experimental Particle Physics
For the past few years my research has focused on solar neutrino data collected with the Sudbury Neutrino Observatory (SNO). We have proven with SNO that neutrinos have mass and we have measured some of the fundamental parameters connecting neutrino mass and flavour states.

Following on the success of SNO, the SNOLAB facility for underground particle physics research has been funded with construction nearing completion by the end of 2007.

My investigations into the properties of neutrinos continues as a collaborator on the Enriched Xenon Observatory (EXO). The EXO detector acts as both a Time Projection Chamber (TPC) and a scintillation counter used to search for the neutrinoless double beta decay of 136Xe. Such decays can only occur if neutrinos are their own anti-particle (Majorana) and a positive signal would provide a first measurement of the neutrino mass scale.

I am also a member of the Dark matter Experiment with Argon Pulse shape discrimation (DEAP). This is a liquid argon scintillation counter designed for low background, low energy threshold detection of nuclear recoil events consistent with WIMP dark matter at the Earth. More than 85% of the universe consists of some unknown dark matter and a direct detection of dark matter particles would be one of the most exciting discoveries of recent times.

© Department of Physics, 3302 Herzberg Building, Tel: (613) 520-4320, Fax: (613) 520-4061, Email: physics[at]carleton.ca