Grant: Canada Excellence Research Chairs
McGill University
$1,051,530.00
Transient Astrophysics
FY 2024-25
Summary
The Universe is not static but continuously changing, even on human-observable timescales. Stars die in supernova explosions, black holes are fed by the gas around them, and neutron stars crash into each other. Transient astrophysics, also called time-domain astronomy, is the study of how astronomical objects change with time. Compared with a static view of the Universe, it provides a new dimension for understanding the grand story of how galaxies, stars, planets, and eventually life are formed. Transient astrophysics is driven by discovery. We aim to uncover new astrophysical phenomena and objects that challenge existing theory, lead to new hypotheses, and provide novel scientific applications.
A recent outstanding example is the discovery of `fast radio bursts'. These radio flashes come from billions of lightyears away in distant galaxies. Their origins are one of the biggest mysteries in astrophysics. We aim to decipher the nature of fast radio bursts, and to use them to reveal the otherwise invisible gas between stars and galaxies. Fast radio bursts encode the history of their journey to Earth; they probe the intervening gas, the fuel for new stars, in unique and powerful ways. This will show us how stars and galaxies evolve over cosmic time. We also aim to explore the skies as never done before, to search for novel astrophysical phenomena that give insight into the Universe's extremes.
To achieve this, we need to construct ground-breaking radio telescopes that can continuously scan wide swaths of the sky, identify ephemeral signals in real-time, and pin-point the source's position with exquisite precision. This is challenging because the scientifically interesting astronomical signals constitute only one millionth of the torrent of data streaming through the telescope. We will greatly expand the Canadian CHIME telescope, creating a network of radio antennas that spans the continent and discovers dozens of precisely localised fast radio bursts per day. Each of these signals provides a view of the Universe's structure in one direction. Combined, the thousands of fast radio bursts that we will discover and localise will give an unprecedented 3-D map of the Universe.
The fast radio burst phenomenon came as a huge surprise, but we now know that we are only seeing the tip of the iceberg of a much larger population of astronomical signals that can transform our understanding of astrophysics and cosmology. We will capitalise on this opportunity.
Program
Canada Excellence Research ChairsCanada Excellence Research Chairs (linked with high confidence)
Recipient
Location
Quebec, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
CERC-2022-00009
Name nom
Hessels, Jason
Department département
Anton Pannekoek Institute for Astronomy - University of Amsterdam
Organization id
61
Institution établissement
McGill University
Province en
Québec
Province fr
Québec
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2024
Competition year année de concours
2022
Award amount
1051530
Program id
CERC
Program name en
Canada Excellence Research Chairs
Program name fr
Programme des chaires d'excellence en recherche du Canada
Group en
DISCOVERY RESEARCH
Group fr
RECHERCHE AXÉE SUR LA DÉCOUVERTE
Committee code
9996
Committee name en
Canada Excellence Research Chairs Selection Committee
Committee name fr
Comité de sélection des Chaires d’excellence en recherche du Canada
Area of application code
9999
Area of application group en
Not available
Area of application group fr
Non disponible
Area of application en
Not available
Area of application fr
Non disponible
Research subject code
9999
Research subject group en
Not available
Research subject group fr
Non disponible
Research subject en
Not available
Research subject fr
Non disponible
Field of research list codes
RDF1010211; RDF1030103; RDF1030104; RDF1030208
Field of research list names en
Numerical analysis;Astronomical and space instrumentation (including atmospheric observation);Cosmology and extragalactic astronomy;High-energy astrophysics and cosmic rays
Field of research list names fr
Analyse numérique;Instrumentation pour l'astronomie et l'espace (y compris l'observation de l'atmosphère);Cosmologie et astronomie extragalactique;Astrophysique des hautes énergies et rayons cosmiques
Socioeconomic objective list codes
RDS10301
Socioeconomic objective list names en
Scientific exploration of space
Socioeconomic objective list names fr
Exploration scientifique de l'espace
Application title
Transient Astrophysics
Keywords
Radio telescope instrumentation; Techniques for searching for FRBs; FRB progenitors; Pulsars; Magnetars; Observational cosmology; High-energy astrophysics; Astrophysical transients; Fast radio bursts (FRBs); Big data in astronomy
Application summary
The Universe is not static but continuously changing, even on human-observable timescales. Stars die in supernova explosions, black holes are fed by the gas around them, and neutron stars crash into each other. Transient astrophysics, also called time-domain astronomy, is the study of how astronomical objects change with time. Compared with a static view of the Universe, it provides a new dimension for understanding the grand story of how galaxies, stars, planets, and eventually life are formed. Transient astrophysics is driven by discovery. We aim to uncover new astrophysical phenomena and objects that challenge existing theory, lead to new hypotheses, and provide novel scientific applications.
A recent outstanding example is the discovery of `fast radio bursts'. These radio flashes come from billions of lightyears away in distant galaxies. Their origins are one of the biggest mysteries in astrophysics. We aim to decipher the nature of fast radio bursts, and to use them to reveal the otherwise invisible gas between stars and galaxies. Fast radio bursts encode the history of their journey to Earth; they probe the intervening gas, the fuel for new stars, in unique and powerful ways. This will show us how stars and galaxies evolve over cosmic time. We also aim to explore the skies as never done before, to search for novel astrophysical phenomena that give insight into the Universe's extremes.
To achieve this, we need to construct ground-breaking radio telescopes that can continuously scan wide swaths of the sky, identify ephemeral signals in real-time, and pin-point the source's position with exquisite precision. This is challenging because the scientifically interesting astronomical signals constitute only one millionth of the torrent of data streaming through the telescope. We will greatly expand the Canadian CHIME telescope, creating a network of radio antennas that spans the continent and discovers dozens of precisely localised fast radio bursts per day. Each of these signals provides a view of the Universe's structure in one direction. Combined, the thousands of fast radio bursts that we will discover and localise will give an unprecedented 3-D map of the Universe.
The fast radio burst phenomenon came as a huge surprise, but we now know that we are only seeing the tip of the iceberg of a much larger population of astronomical signals that can transform our understanding of astrophysics and cosmology. We will capitalise on this opportunity.