Grant: Subatomic Physics Envelope - Individual
Laurentian University of Sudbury
$40,000.00
PICASSO group at laurentian university
EF 2007-08
Résumé
Although astronomical and astrophysical observations of the Universe indicate that dark matter is everywhere, its nature represents a problem for modern science that has not been solved yet. Nevertheless, there is a strong belief among physicists that dark matter is made of elementary particles.Observations indicate that dark matter forms halos that involve spiral galaxies like ours (the Milky Way). Scientists believe that dark matter particles are zooming around in the Milky Way in such a number that 10 million particles would pass through the cap of a soda bottle every second. Many experiments are under way to detect these particles but no one has been able to indisputably claim the detection of dark matter particles.The elementary particles presently known and described in the Standard Model of Particle Physics do not have the properties that scientists believe dark matter particles must have. These properties include i-) No electromagnetic interaction with ordinary matter (that is why they are dark); ii-) creates a gravitational pull (that is why we know they are there); iii-) a feeble interaction with ordinary matter. It is this feeble interaction of dark matter particles with ordinary matter what we hope will reveal dark matter's nature.The PICASSO (Project In Canada to Search for Super Symmetric Objects) dark matter search experiment has recently achieved one of the best performances in the search for dark matter. The PICASSO Collaboration, which uses the superheated droplet technique, develops its own detectors, which allows for a low cost of production and operation. The PICASSO Collaboration is now developing and installing larger detectors at SNOLAB and refining its technique in order to maximize even more our chance of detecting dark matter particles. The next generation of dark matter search experiments is going to be more sensitive, i.e., will be able to detect dark matter particles even if their interaction with ordinary matter is 1,000 times weaker than the levels we can detect today. The PICASSO Collaboration is in an excellent position to get there first.
Programme
Subatomic Physics Envelope - Individual
Bénéficiaire
Emplacement
Ontario, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
341329-2007
Name nom
Wichoski, Ubi
Department département
Physics
Organization id
26
Institution établissement
Laurentian University of Sudbury
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2007
Competition year année de concours
2007
Award amount
40000
Program id
SAPIN
Program name en
Subatomic Physics Envelope - Individual
Program name fr
Enveloppe de physique subatomique - Individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
19
Committee name en
Subatomic Physics
Committee name fr
Physique subatomique
Area of application code
1202
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Physical sciences
Area of application fr
Sciences physiques
Research subject code
3104
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Particle physics
Research subject fr
Physique des particules
Partie
1
Nb partie
1
Application title
PICASSO group at laurentian university
Keyword
NA
Application summary
Although astronomical and astrophysical observations of the Universe indicate that dark matter is everywhere, its nature represents a problem for modern science that has not been solved yet. Nevertheless, there is a strong belief among physicists that dark matter is made of elementary particles.Observations indicate that dark matter forms halos that involve spiral galaxies like ours (the Milky Way). Scientists believe that dark matter particles are zooming around in the Milky Way in such a number that 10 million particles would pass through the cap of a soda bottle every second. Many experiments are under way to detect these particles but no one has been able to indisputably claim the detection of dark matter particles.The elementary particles presently known and described in the Standard Model of Particle Physics do not have the properties that scientists believe dark matter particles must have. These properties include i-) No electromagnetic interaction with ordinary matter (that is why they are dark); ii-) creates a gravitational pull (that is why we know they are there); iii-) a feeble interaction with ordinary matter. It is this feeble interaction of dark matter particles with ordinary matter what we hope will reveal dark matter's nature.The PICASSO (Project In Canada to Search for Super Symmetric Objects) dark matter search experiment has recently achieved one of the best performances in the search for dark matter. The PICASSO Collaboration, which uses the superheated droplet technique, develops its own detectors, which allows for a low cost of production and operation. The PICASSO Collaboration is now developing and installing larger detectors at SNOLAB and refining its technique in order to maximize even more our chance of detecting dark matter particles. The next generation of dark matter search experiments is going to be more sensitive, i.e., will be able to detect dark matter particles even if their interaction with ordinary matter is 1,000 times weaker than the levels we can detect today. The PICASSO Collaboration is in an excellent position to get there first.