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Gravitational waves from binary supermassive black holes missing in pulsar observations Paul Lasky, on behalf of the Shannon et al., 2015 (Science)

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Page 1: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Gravitational waves from binary supermassive black holes

missing in pulsar observations

Paul Lasky, on behalf of the

Shannon et al., 2015 (Science)

Page 2: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Paul Lasky

LIGO

Pulsar Timing! Arrays

๏ Supermassive black hole binaries • stochastic background!• individual binaries !

๏ Cosmic Strings !

๏ Relics from Inflation

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Page 3: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Supermassive black hole mergers๏ Assume all galaxies host a SMBH ๏ Use observed BH-Galaxy mass relations ๏ Assume BH merger rate traces galaxy merger rate ๏ Assume GW dominated mergers (circular, …) ๏ … ๏ Sum up contribution from all SMBHs mergers in Universe

Page 4: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Paul Lasky

๏ all binaries have circular orbits ๏ all binaries driven through band by GW emission

shared assumptions

Page 5: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Tim

e-of

-arri

val r

esid

ual (μs)

Time (yr)

J1909-3744

J0437-4715

J1713+0747

J1744-1134

Paul Lasky

Page 6: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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PSR J1909-3744 Paul Lasky

RMS residuals =102 ns

RMS residuals = 160 ns3 improvements

• longer baseline (+3yr) !

• discrete phase offsets !

• short λ obs. only

Colours are different telescope

backends

Page 7: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Shannon et al. !(2013)

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Paul Lasky

Page 8: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Shannon et al.! (2015) Shannon et al. !

(2013)

80.09Pmodel 0.06 0.002 0.005

Paul Lasky

Page 9: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Arzoumanian et al. (2015; NANOGrav)

Astrophysical !Inference

๏ Black hole mass function at z ~ 2?

๏ Galaxy merger rate? ๏ Environmental factors: stars, gas, …

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Paul Lasky

Page 10: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Paul Lasky

Is the final parsec problem solved?Stalled evolution:!• many binary systems • rogue, isolated BHs from 3-

body interactions

sciencedaily.com

Page 11: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

The Environment

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Paul Lasky

Sesana (2013)

Stars: Gas:

GWs: Circular inspiral

Where is the ‘knee’?

• gas/stellar density in galactic cores? • actual masses of supermassive BHs? • ….

need to understand:

Page 12: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

The Environment

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Paul Lasky

Ravi et al. (2014)

non-zero eccentricities

GWs circularise orbitssome other effects drive eccentricity up:

e.g., retrograde circumbinary accretion, …

Enoki & Nagashima (2007)

Page 13: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

What Next?

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Paul Lasky

keep observing…!(high frequency, high cadence, best pulsars)

future telescopes!SKA, FAST, …

single sourcese.g., Graham et al. (2015)!

Catalina Real-time Transient Survey

stra

in a

mpl

itude

log(freq [Hz])

combined datasets

Page 14: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

Conclusions

๏ PPTA currently doing cosmology with non-detections!!!

!

๏ Our understanding of galaxy/black hole evolutionneeds updating

Paul Lasky

Page 15: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Extra Slides

Page 16: Gravitational waves from binary supermassive …users.monash.edu.au/~plasky/files/talks/PPTA_GWB_limit.pdf · Gravitational waves from binary supermassive black holes missing in pulsar

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Paul Lasky