Grant: Discovery Grants Program - Individual
Saint Mary's University
$27,000.00
New insights into galaxy formation and evolution
EF 2015-16
Résumé
Buried within our galactic backyard is a treasure trove of information about how our galaxy, the Milky Way, formed and evolved. The field of ""galactic archaeology"" sets out to uncover and decipher the implications of this information both for our galaxy and galaxy formation in general. In the next decade, galactic archaeology is about to undergo a revolution as the European Space Agency's Gaia mission will provide exquisite new observations of the stellar positions of over a billion stars and true motions of tens of millions. Combined with upcoming surveys of the chemical signatures of stars (stars with similar chemical signatures were likely formed together) we will then be able to piece together their evolution back in time. The first part of my research program outlines a series of simulations on parallel computers that will introduce new levels of fidelity into our studies of galactic archaeology, and enable us to model upcoming data from the Gaia survey (and others) with great precision. Step-by-step I will increase physical complexity so as to eventually include all the dominant physical processes present in the Milky Way.
The second part of the research program will focus on how black holes, once thought to be largely irrelevant in the process of galaxy formation, can actually directly determine the evolution of the largest galaxies. Due to the presence of an accretion disk around them, black holes actually liberate and return vast amounts of energy to their surrounding galaxy. But describing this process is immensely difficult. Even supermassive black holes, with masses tens of millions of times that of the Sun, are tiny compared to the overall size of a galaxy - the ratio is akin to a grain of sand and the entire Earth. The research outlined in this proposal will improve our modelling of this process by adding greater physical complexity and also allowing us to follow the energy that flows out from black holes to large radii where it interacts with the rest of the galaxy.
Programme
Discovery Grants Program - Individual
Bénéficiaire
Emplacement
Nova Scotia, Canada
Type de bénéficiaire
Academia
Type
Grant
Source
NSERC's Awards Data
Tel que publié
Application id
341284-2013
Name nom
Thacker, Robert
Department département
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
2015
Competition year année de concours
2013
Award amount
27000
Program id
RGPIN
Program name en
Discovery Grants Program - Individual
Program name fr
Programme de subventions à la découverte - individuelles
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
1505
Committee name en
Physics
Committee name fr
Physique
Area of application code
802
Area of application group en
Information and communication services
Area of application group fr
Services d'information et de télécommunications
Area of application en
Information systems and technology
Area of application fr
Systèmes d'information et technologie de l'information
Research subject code
3200
Research subject group en
Astronomy and astrophysics
Research subject group fr
Astronomie et astrophysique
Research subject en
Astronomy and astrophysics
Research subject fr
Astronomie et astrophysique
Partie
3
Nb partie
5
Application title
New insights into galaxy formation and evolution
Keyword
NSERC
Application summary
Buried within our galactic backyard is a treasure trove of information about how our galaxy, the Milky Way, formed and evolved. The field of ""galactic archaeology"" sets out to uncover and decipher the implications of this information both for our galaxy and galaxy formation in general. In the next decade, galactic archaeology is about to undergo a revolution as the European Space Agency's Gaia mission will provide exquisite new observations of the stellar positions of over a billion stars and true motions of tens of millions. Combined with upcoming surveys of the chemical signatures of stars (stars with similar chemical signatures were likely formed together) we will then be able to piece together their evolution back in time. The first part of my research program outlines a series of simulations on parallel computers that will introduce new levels of fidelity into our studies of galactic archaeology, and enable us to model upcoming data from the Gaia survey (and others) with great precision. Step-by-step I will increase physical complexity so as to eventually include all the dominant physical processes present in the Milky Way.
The second part of the research program will focus on how black holes, once thought to be largely irrelevant in the process of galaxy formation, can actually directly determine the evolution of the largest galaxies. Due to the presence of an accretion disk around them, black holes actually liberate and return vast amounts of energy to their surrounding galaxy. But describing this process is immensely difficult. Even supermassive black holes, with masses tens of millions of times that of the Sun, are tiny compared to the overall size of a galaxy - the ratio is akin to a grain of sand and the entire Earth. The research outlined in this proposal will improve our modelling of this process by adding greater physical complexity and also allowing us to follow the energy that flows out from black holes to large radii where it interacts with the rest of the galaxy.