Grant: Research Tools and Instruments - Category 1 (<$150,000)
University of British Columbia
$142,876.00
Focal plane electronics for the CHIME pathfinder instrument.
FY 2011-12
Summary
We are requesting funds to build receiver electronics for a novel, one-dimensional Fourier transform telescope which we will install on the radio-quiet campus of the Dominion Radio Astrophysical Observatory. This instrument is a pathfinder experiment for a baryon acoustic oscillation experiment called CHIME.
The most surprising discovery in cosmology in recent times, awarded the 2011 Nobel Prize in Physics, is the accelerating expansion of the Universe. This either signals that a previously unknown component called Dark Energy dominates the energy density of the Universe, or that our understanding of gravity on large scales is incorrect. The implications for fundamental physics are profound, and advancing our understanding requires new, higher-quality data. More precise observations of expansion history would better constrain the physics of Dark Energy. Measurement through cosmic time of ""baryon acoustic oscillations"" (BAO), the remnant of sound waves in the primordial plasma, provides the most reliable probe of expansion history. A novel technique for mapping matter, called hydrogen intensity (HI) mapping, has recently been demonstrated by a team led by co-applicant Pen, and allows one to measure the BAO signal as a function of redshift without the cumbersome intermediate step of detecting individual galaxies. This is what CHIME is designed to do.
The full CHIME instrument will survey half the sky and reach definitive sensitivity in 2 years of observing. The pathfinder instrument, with 10% of the ultimate collecting area, will still be sensitive enough to produce the largest volume hydrogen redshift survey to date. With it we will advance the intensity mapping technique, demonstrate galactic foreground suppression, and probe the matter power spectrum. The electronics requested here will allow us to build the CHIME pathfinder and will poise Canada to play a leading role in Dark Energy research.
Program
Research Tools and Instruments - Category 1 (<$150,000)
Recipient
Location
British Columbia, Canada
Recipient Type
Academia
Type
Grant
Source
NSERC's Awards Data
As published
Application id
423969-2012
Name nom
Halpern, Mark
Department département
Physics and Astronomy
Organization id
2
Institution établissement
University of British Columbia
Province en
British Columbia
Province fr
Colombie-Britannique
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2011
Competition year année de concours
2012
Award amount
142876
Program id
EQPEQ
Program nane en
Research Tools and Instruments - Category 1 (<$150,000)
Program name fr
Outils et instruments de recherche - catégorie 1 (<150 000$)
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
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
Partie
1
Nb partie
1
Application title
Focal plane electronics for the CHIME pathfinder instrument.
Keyword
NSERC
Application summary
We are requesting funds to build receiver electronics for a novel, one-dimensional Fourier transform telescope which we will install on the radio-quiet campus of the Dominion Radio Astrophysical Observatory. This instrument is a pathfinder experiment for a baryon acoustic oscillation experiment called CHIME.
The most surprising discovery in cosmology in recent times, awarded the 2011 Nobel Prize in Physics, is the accelerating expansion of the Universe. This either signals that a previously unknown component called Dark Energy dominates the energy density of the Universe, or that our understanding of gravity on large scales is incorrect. The implications for fundamental physics are profound, and advancing our understanding requires new, higher-quality data. More precise observations of expansion history would better constrain the physics of Dark Energy. Measurement through cosmic time of ""baryon acoustic oscillations"" (BAO), the remnant of sound waves in the primordial plasma, provides the most reliable probe of expansion history. A novel technique for mapping matter, called hydrogen intensity (HI) mapping, has recently been demonstrated by a team led by co-applicant Pen, and allows one to measure the BAO signal as a function of redshift without the cumbersome intermediate step of detecting individual galaxies. This is what CHIME is designed to do.
The full CHIME instrument will survey half the sky and reach definitive sensitivity in 2 years of observing. The pathfinder instrument, with 10% of the ultimate collecting area, will still be sensitive enough to produce the largest volume hydrogen redshift survey to date. With it we will advance the intensity mapping technique, demonstrate galactic foreground suppression, and probe the matter power spectrum. The electronics requested here will allow us to build the CHIME pathfinder and will poise Canada to play a leading role in Dark Energy research.