Grant: Subatomic Physics Envelope - Research Tools and Instruments
Saint Mary's University
$127,109.00
Strip Scintillator Array with ultra-FAst timing for Rare Isotope study (SAFARI)
EF 2022-23
Résumé
Nuclei, the core of all visible matter, embody the beauty of nature's strong force binding the building blocks, protons and into a wide variety of complex many body systems. Most of the long--lived nuclei occurring naturally on earth have a nearly balanced ratio of neutrons to protons. Rare isotopes with a large neutron to proton asymmetry are created in some of nature's most exotic environments that are rich in neutrons, such as neutron stars and supernovae, or rich in protons, such a accretion disks on the surface of a neutron star. These neutron--rich or proton--rich isotopes therefore, open before us a wealth of new knowledge on the fundamentals of how nature organizes such systems and their role in creation of majority of the heavy elements around us. Signature of such element synthesis was recently seen in one of nature's most cataclysmic events, in the merger of two neutron stars. This proposal aims to develop ultra-fast-timing plastic scintillator arrays that are necessary to identify the rare isotopes produced in our laboratories. Their production takes place with nuclear reactions, such as fragmentation or fission in a few specialized accelerator facilities in the world among which the facility at GSI in Germany provides highest energy beams of the rare isotopes. Using the relativistic rare isotope beams we aim to unravel how the neutrons are distributed in such np asymmetric conditions. This provides guidance to characterize the behavior of neutron--rich environments of our Universe. This also brings new information on the nuclear (strong) force and how that governs the arrangement, i.e. shell structure, and properties of the rare isotopes. The properties of these isotopes determine how their reactions and decays drive the creation of most of the heavy elements in nature.
Programme
Subatomic Physics Envelope - Research Tools and Instruments
Bénéficiaire
Emplacement
Nova Scotia, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
SAPEQ-2022-00004
Name nom
Kanungo, Rituparna
Department département
Astronomy and Physics - Astronomy and Physics
Organization id
85
Institution établissement
Saint Mary's University
Province en
Nova Scotia
Province fr
Nouvelle-Écosse
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2022
Competition year année de concours
2022
Award amount
127109
Program id
SAPEQ
Program name en
Subatomic Physics Envelope - Research Tools and Instruments
Program name fr
Enveloppe de physique subatomique - Outils et instruments de recherche
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR LA DÉCOUVERTE
Committee code
19
Committee name en
Subatomic Physics
Committee name fr
Physique subatomique
Area of application code
1200
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Advancement of knowledge
Area of application fr
Avancement des connaissances
Research subject code
3100
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Physics
Research subject fr
Physique
Installment
inst:1
Partie
1
Nb partie
1
Application title
Strip Scintillator Array with ultra-FAst timing for Rare Isotope study (SAFARI)
Application summary
Nuclei, the core of all visible matter, embody the beauty of nature's strong force binding the building blocks, protons and into a wide variety of complex many body systems. Most of the long--lived nuclei occurring naturally on earth have a nearly balanced ratio of neutrons to protons. Rare isotopes with a large neutron to proton asymmetry are created in some of nature's most exotic environments that are rich in neutrons, such as neutron stars and supernovae, or rich in protons, such a accretion disks on the surface of a neutron star. These neutron--rich or proton--rich isotopes therefore, open before us a wealth of new knowledge on the fundamentals of how nature organizes such systems and their role in creation of majority of the heavy elements around us. Signature of such element synthesis was recently seen in one of nature's most cataclysmic events, in the merger of two neutron stars. This proposal aims to develop ultra-fast-timing plastic scintillator arrays that are necessary to identify the rare isotopes produced in our laboratories. Their production takes place with nuclear reactions, such as fragmentation or fission in a few specialized accelerator facilities in the world among which the facility at GSI in Germany provides highest energy beams of the rare isotopes. Using the relativistic rare isotope beams we aim to unravel how the neutrons are distributed in such np asymmetric conditions. This provides guidance to characterize the behavior of neutron--rich environments of our Universe. This also brings new information on the nuclear (strong) force and how that governs the arrangement, i.e. shell structure, and properties of the rare isotopes. The properties of these isotopes determine how their reactions and decays drive the creation of most of the heavy elements in nature.