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Peculiar Velocities in Supernova Cosmology Bryony Martin MSc, Department of Astronomy, University of Cape Town Supervised by: Dr Kurt van der Heyden & Prof Bruce Bassett SKA SA Postgraduate Bursary Conference, November 2011 Kessler, et al. 2009

Bryony Martin SKA Conference 2011

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Page 1: Bryony Martin SKA Conference 2011

Peculiar Velocities in Supernova Cosmology

Bryony MartinMSc, Department of Astronomy, University of Cape Town

Supervised by: Dr Kurt van der Heyden & Prof Bruce Bassett

SKA SA Postgraduate Bursary Conference, November 2011

Kessler, et al. 2009

Page 2: Bryony Martin SKA Conference 2011

Peculiar Velocities in Supernova Cosmology2 Bryony Martin 2011

Peculiar velocitiesAdditional motions specific to individual galaxies

• Recession velocity due to Hubble flow

• Peculiar velocity due to matter distribution of local environment

– baryonic and dark matter

Recession velocity

Peculiar velocity

Overdensity

LINE OF SIGHT

radial

transverse

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Type Ia supernovaeThe standard candles of the universe

Kim, et al. 1997

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Supernova cosmologyCalculating constraints on cosmological parameters

Kessler, et al. 2009Kessler, et al. 2009

Page 5: Bryony Martin SKA Conference 2011

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Supernova cosmology with peculiar velocitiesPeculiar velocities induce Doppler effects in supernova observations

Kessler, et al. 2009Doppler shifting

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Peculiar Velocities in Supernova Cosmology6 Bryony Martin 2011

Supernova cosmology with peculiar velocitiesPeculiar velocities induce Doppler effects in supernova observations

Kessler, et al. 2009Doppler shifting

Inaccurate best-fit cosmology

INACCURATE PARAMETER

CONSTRAINTS

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Peculiar Velocities in Supernova Cosmology7 Bryony Martin 2011

Simulation dataSimulated galaxies with explicit velocity information

Kitzbichler & White, 2007

www.mpa-garching.mpg.de

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Peculiar Velocities in Supernova Cosmology8 Bryony Martin 2011

Simulated galaxiesMock survey galaxy catalogues showing structure

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Supernova ratesUsing galaxy properties to predict the presence of type Ia supernovae

Mannucci et al, 2005

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Simulated Type Ia SupernovaeSupernova dataset with known peculiar velocities

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Hubble diagramConstructed using simulated supernova data

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Shifts in Ωm for various maximum redshifts

Average shifts in Ωm are within 1σ

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Shifts in H0 for various maximum redshifts

Average shifts in H0 are ~1σ

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Calculated values of Ωm using true and observed redshifts

Calculated values are 1-2σ from the fiducial value of Ωm

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Peculiar Velocities in Supernova Cosmology15 Bryony Martin 2011

Calculated values of H0 using true and observed redshifts

Calculated values using observed redshifts are 2σ less than the fiducial value of H0

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Peculiar Velocities in Supernova Cosmology16 Bryony Martin 2011

Summary

RESULTS Simulated type Ia supernova dataset with peculiar velocity information

• Parameter estimates from simulated Hubble diagrams using both cosmological and observed redshifts

• Measured shifts in parameters which are roughly of the order of 1σ