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Grant: Discovery Launch Supplement

York University

$12,500.00

Revealing the nature of Fast Radio Bursts and unlocking their potential as probes of the Universe

EF 2024-25

Résumé
My proposed research program is to develop and utilize novel Canadian radio telescopes to perform ground-breaking research on transient phenomena in astronomy, such as Fast Radio Bursts (FRBs).  Astrophysical transients (transients) are sources that vary on human timescales (nano-seconds to years) that are detected across the electromagnetic spectrum by telescopes. Since transients change on rapid timescales it is believed they must come from some of the most extreme physical environments in the Universe. FRBs are probably the most exciting recently discovered transient. They are nano- to milli-second-long flashes of radio light of as-yet unknown origin that come from far outside of our Milky Way Galaxy. FRBs are both an exciting cosmic mystery and show great promise as probes of extreme physics and the structure of the cosmos. Because of their brevity and origins at extreme distances they must arise from the most highly magnetized and/or relativistic phenomena in the universe. They also carry with them a record of the matter between Earth and their sources through the effect of chromatic dispersion. Chromatic dispersion causes radio bursts to arrive at different times for different frequencies of radio light, and the amount of this time difference is directly related to the amount of electrons encountered between the signal's source and our planet. FRBs are thus powerful new probes of cosmic structure. My objectives are: (i) to uncover the nature of the physical engines that power FRBs, (ii) unlock the potential of FRBs as cosmic probes, and (iii) search for and discover other new fast transient phenomena. These objectives will be enabled by Canadian built instruments: the Canadian Hydrogen Intensity Mapping Experiment (CHIME) and the Canadian Hydrogen Observatory and Radio-transient Detector (CHORD). CHIME has already revolutionized the FRB field by discovering thousands of such events (compared to dozens previously known). The next breakthroughs will come from CHIME/FRB Outriggers and CHORD. CHIME/FRB Outriggers will enable us to pinpoint the galaxies that FRBs come from leading to a profound advancement in understanding of the environments where FRBs live. CHORD will provide an order of magnitude larger discovery rate of FRBs and their host galaxies at even further distances from CHIME, thus propelling us into the age of FRBs as probes of cosmic structure. Results from my research will advance knowledge on transient astrophysical phenomena, especially FRBs. These advances can be used for further research in the field and my development of the novel software infrastructure that powers CHIME, its Outriggers and CHORD, will establish Canada as a global leader in this area. Additionally, I will provide training to students and others in my research program that will give them highly transferable technical skill sets which will benefit employment in Canada both in academia and industry.
Programme
Discovery Launch Supplement
Bénéficiaire
Emplacement
Ontario, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data

Tel que publié

Application id
DGECR-2024-00046
Name nom
Scholz, Paul
Department département
Physics and Astronomy
Organization id
38
Institution établissement
York University
Province en
Ontario
Province fr
Ontario
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2024
Competition year année de concours
2024
Award amount
12500
Program id
DGECR
Program name en
Discovery Launch Supplement
Program name fr
Supplément Tremplin vers la découverte
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR LA DÉCOUVERTE
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
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
3204
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Extra galactic and cosmology
Research subject fr
Extra-galactique et cosmologie
Field of research list names en
Not available
Field of research list names fr
Non disponible
Socioeconomic objective list names en
Not available
Socioeconomic objective list names fr
Non disponible
Application title
Revealing the nature of Fast Radio Bursts and unlocking their potential as probes of the Universe
Keywords
radio astronomy; astrophysical transients; fast radio bursts; astronomy surveys; time-domain astronomy; high-energy astrophysics; magnetars; neutron stars
Application summary
My proposed research program is to develop and utilize novel Canadian radio telescopes to perform ground-breaking research on transient phenomena in astronomy, such as Fast Radio Bursts (FRBs).  Astrophysical transients (transients) are sources that vary on human timescales (nano-seconds to years) that are detected across the electromagnetic spectrum by telescopes. Since transients change on rapid timescales it is believed they must come from some of the most extreme physical environments in the Universe. FRBs are probably the most exciting recently discovered transient. They are nano- to milli-second-long flashes of radio light of as-yet unknown origin that come from far outside of our Milky Way Galaxy. FRBs are both an exciting cosmic mystery and show great promise as probes of extreme physics and the structure of the cosmos. Because of their brevity and origins at extreme distances they must arise from the most highly magnetized and/or relativistic phenomena in the universe. They also carry with them a record of the matter between Earth and their sources through the effect of chromatic dispersion. Chromatic dispersion causes radio bursts to arrive at different times for different frequencies of radio light, and the amount of this time difference is directly related to the amount of electrons encountered between the signal's source and our planet. FRBs are thus powerful new probes of cosmic structure. My objectives are: (i) to uncover the nature of the physical engines that power FRBs, (ii) unlock the potential of FRBs as cosmic probes, and (iii) search for and discover other new fast transient phenomena. These objectives will be enabled by Canadian built instruments: the Canadian Hydrogen Intensity Mapping Experiment (CHIME) and the Canadian Hydrogen Observatory and Radio-transient Detector (CHORD). CHIME has already revolutionized the FRB field by discovering thousands of such events (compared to dozens previously known). The next breakthroughs will come from CHIME/FRB Outriggers and CHORD. CHIME/FRB Outriggers will enable us to pinpoint the galaxies that FRBs come from leading to a profound advancement in understanding of the environments where FRBs live. CHORD will provide an order of magnitude larger discovery rate of FRBs and their host galaxies at even further distances from CHIME, thus propelling us into the age of FRBs as probes of cosmic structure. Results from my research will advance knowledge on transient astrophysical phenomena, especially FRBs. These advances can be used for further research in the field and my development of the novel software infrastructure that powers CHIME, its Outriggers and CHORD, will establish Canada as a global leader in this area. Additionally, I will provide training to students and others in my research program that will give them highly transferable technical skill sets which will benefit employment in Canada both in academia and industry.