Built on

C. P. L. Berry, S. A. Hughes, C. F. Sopuerta, A. J. K. Chua, A. Heffernan, K. Holley-Bockelmann, D. P. Mihaylov, M. C. Miller, and A. Sesana, The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy (2019), arXiv:1903.03686 [astro-ph.HE]
Original
1903
Earlier work this paper cites.
Y.-F. Jiang, O. Blaes, J. Stone, and S. W. Davis, Global Radiation Magneto-hydrodynamic Simulations of Sub-Eddington Accretion Disks around Supermassive Black Holes (2019a), arXiv:1904.01674 [astro-ph.HE]
Original
1904
Earlier work this paper cites.
O. A. Hannuksela, K. C. Y. Ng, and T. G. F. Li, Extreme dark matter tests with extreme mass ratio inspirals, Phys. Rev. D 102
Original
1906
Earlier work this paper cites.
J. Jiang, A. C. Fabian, T. Dauser, L. Gallo, J. A. Garcia, E. Kara, M. L. Parker, J. A. Tomsick, D. J. Walton, and C. S. Reynolds, High Density Reflection Spectroscopy – II. The density of the inner black hole accretion disc in AGN, Mon. Not. Roy. Astron. Soc. 489
Original
1908
Earlier work this paper cites.
M. MacLeod and D. N. C. Lin, The Effect of Star-Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events, ApJ 889
Original
1909
Earlier work this paper cites.
O. Burke, J. R. Gair, and J. Simón, Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform, Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
A. J. Dittmann and M. C. Miller, Star formation in accretion discs and SMBH growth, Mon. Not. Roy. Astron. Soc. 493
Original
1911
Earlier work this paper cites.
C. E. Scardoni, G. P. Rosotti, G. Lodato, and C. J. Clarke, Type II migration strikes back - an old paradigm for planet migration in discs, MNRAS 492
Original
1912
Earlier work this paper cites.
N. I. Shakura and R. A. Sunyaev, Black holes in binary systems. Observational appearance, Astron. Astrophys. 24
1973
Earlier work this paper cites.
A. P. Lightman and D. M. Eardley, Black Holes in Binary Systems: Instability of Disk Accretion, Astrophys. J. Lett. 187
1974
Earlier work this paper cites.
J. M. Bardeen and J. A. Petterson, The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes, Astrophys. J. Lett. 195
1975
Earlier work this paper cites.
N. I. Shakura and R. A. Sunyaev, A Theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars, Mon. Not. Roy. Astron. Soc. 175
1976
Earlier work this paper cites.
G. S. Bisnovatyi-Kogan and S. I. Blinnikov, Disk accretion onto a black hole at subcritical luminosity., A&A 59
1977
Earlier work this paper cites.
T. Piran, The role of viscosity and cooling mechanisms in the stability of accretion disks., ApJ 221
1978
Earlier work this paper cites.
P. Goldreich and S. Tremaine, Disk-satellite interactions., ApJ 241
1980
Earlier work this paper cites.
P. Sakimoto and F. Coroniti, Accretion disk models for qsos and active galactic nuclei - the role of magnetic viscosity, Astrophys. J. 247
1981
Earlier work this paper cites.
M. A. Abramowicz, B. Czerny, J. P. Lasota, and E. Szuszkiewicz, Slim accretion disks, Astrophys. J. 332
1988
Earlier work this paper cites.
D. Syer, C. J. Clarke, and M. J. Rees, Star-disc interactions near a massive black hole, MNRAS 250
1991
Earlier work this paper cites.
D. Syer and C. J. Clarke, Satellites in discs: regulating the accretion luminosity, MNRAS 277
1995
Earlier work this paper cites.
Y. Mino, M. Sasaki, and T. Tanaka, Gravitational radiation reaction to a particle motion, Phys. Rev. D 55
1997
Earlier work this paper cites.
T. C. Quinn and R. M. Wald, Axiomatic approach to electromagnetic and gravitational radiation reaction of particles in curved spacetime, Phys. Rev. D 56
1997
Earlier work this paper cites.
C. Cutler, Angular resolution of the LISA gravitational wave detector, Phys. Rev. D 57
1998
Earlier work this paper cites.
E. C. Ostriker, Dynamical friction in a gaseous medium, Astrophys. J. 513
1999
Earlier work this paper cites.
A. Ori and K. S. Thorne, Transition from inspiral to plunge for a compact body in a circular equatorial orbit around a massive, spinning black hole, Phys. Rev. D 62
2000
Earlier work this paper cites.
J. Goodman and R. R. Rafikov, Planetary torques as the viscosity of protoplanetary disks, Astrophys. J. 552
2001
Earlier work this paper cites.
J. Frank, A. King, and D. Raine, Accretion Power in Astrophysics , 3rd ed. (Cambridge University Press, 2002)
2002
Earlier work this paper cites.
H. Tanaka, T. Takeuchi, and W. R. Ward, Three-Dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration, ApJ 565
2002
Earlier work this paper cites.
B. J. Kavanagh, D. A. Nichols, G. Bertone, and D. Gaggero, Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
Y. Levin, Formation of massive stars and black holes in selfgravitating AGN discs, and gravitational waves in LISA band (2003), arXiv:astro-ph/0307084
2003
Earlier work this paper cites.
L. Barack and C. Cutler, LISA capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy, Phys. Rev. D 69
2004
Earlier work this paper cites.
A. Maselli, N. Franchini, L. Gualtieri, and T. P. Sotiriou, Detecting scalar fields with Extreme Mass Ratio Inspirals, Phys. Rev. Lett. 125
Original
2004
Earlier work this paper cites.
A. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, and A. MacFadyen, Evolution of gas disc–embedded intermediate mass ratio inspirals in the L I S A LISA band, Mon. Not. Roy. Astron. Soc. 501
Original
2005
Earlier work this paper cites.
K. Glampedakis and S. Babak, Mapping spacetimes with LISA: Inspiral of a test-body in a ‘quasi-Kerr’ field, Class. Quant. Grav. 23
2006
Earlier work this paper cites.
G. Fabj, S. S. Nasim, F. Caban, K. E. S. Ford, B. McKernan, and J. M. Bellovary, Aligning nuclear cluster orbits with an active galactic nucleus accretion disc, MNRAS 499
Original
2006
Earlier work this paper cites.
R. N. Lang and S. A. Hughes, Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession, Phys. Rev. D 74
2006
Earlier work this paper cites.
J. P. Gardner et al. , The James Webb Space Telescope, Space Sci. Rev. 123
2006
Earlier work this paper cites.
P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals, Class. Quant. Grav. 24
2007
Earlier work this paper cites.
E. Barausse, L. Rezzolla, D. Petroff, and M. Ansorg, Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes, Phys. Rev. D 75
2007
Earlier work this paper cites.
P. Cresswell, G. Dirksen, W. Kley, and R. P. Nelson, On the evolution of eccentric and inclined protoplanets embedded in protoplanetary disks, A&A 473
Original
2007
Earlier work this paper cites.
L. Barack and C. Cutler, Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes, Phys. Rev. D 75
2007
Earlier work this paper cites.

Similar

T. Bogdanovic, C. S. Reynolds, and M. C. Miller, Alignment of the spins of supermassive black holes prior to merger, Astrophys. J. Lett. 661
2007
Cited alongside, same era.
E. Barausse, Relativistic dynamical friction in a collisional fluid, Mon. Not. Roy. Astron. Soc. 382
Original
2007
Cited alongside, same era.
Y. Levin, Starbursts near supermassive black holes: young stars in the Galactic Center, and gravitational waves in LISA band, Mon. Not. Roy. Astron. Soc. 374
2007
Cited alongside, same era.
P. F. Hopkins, G. T. Richards, and L. Hernquist, An Observational Determination of the Bolometric Quasar Luminosity Function, Astrophys. J. 654
2007
Cited alongside, same era.
L. Annulli, V. Cardoso, and R. Vicente, Stirred and shaken: Dynamical behavior of boson stars and dark matter cores, Phys. Lett. B 811
Original

Then

A. J. K. Chua, C. J. Moore, and J. R. Gair, Augmented kludge waveforms for detecting extreme-mass-ratio inspirals, Phys. Rev. D 96
Original
2017
Later among the works it cites.
K. Chamberlain and N. Yunes, Theoretical Physics Implications of Gravitational Wave Observation with Future Detectors, Phys. Rev. D 96
Original
2017
Later among the works it cites.
P. Amaro-Seoane, Relativistic dynamics and extreme mass ratio inspirals, Living Rev. Rel. 21
Original
2018
Later among the works it cites.
K. D. Kanagawa, H. Tanaka, and E. Szuszkiewicz, Radial Migration of Gap-opening Planets in Protoplanetary Disks. I. The Case of a Single Planet, ApJ 861
Original
2018
Later among the works it cites.
J. Aird, A. L. Coil, and A. Georgakakis, X-rays across the galaxy population – II. The distribution of AGN accretion rates as a function of stellar mass and redshift, Mon. Not. Roy. Astron. Soc. 474

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Reading the bibliography…

2022

Probing Accretion Physics with Gravitational Waves

Speri, Lorenzo, Antonelli, Andrea, Sberna, Laura et al.

Understand

Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) offer the opportunity to probe the environments of active galactic nuclei (AGN) through the torques that accretion disks induce on the binary.

Within a Bayesian framework, we study how well such environmental effects can be measured using gravitational wave observations from the Laser Interferometer Space Antenna (LISA).
We focus on the torque induced by planetary-type migration on quasicircular inspirals, and use different prescriptions for geometrically thin and radiatively efficient disks.
We find that LISA could detect migration for a wide range of disk viscosities and accretion rates, for both $\alpha$ and $\beta$ disk prescriptions.

Built on

C. P. L. Berry, S. A. Hughes, C. F. Sopuerta, A. J. K. Chua, A. Heffernan, K. Holley-Bockelmann, D. P. Mihaylov, M. C. Miller, and A. Sesana, The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy (2019), arXiv:1903.03686 [astro-ph.HE]
Original
1903
Earlier work this paper cites.
Y.-F. Jiang, O. Blaes, J. Stone, and S. W. Davis, Global Radiation Magneto-hydrodynamic Simulations of Sub-Eddington Accretion Disks around Supermassive Black Holes (2019a), arXiv:1904.01674 [astro-ph.HE]
Original
1904
Earlier work this paper cites.
O. A. Hannuksela, K. C. Y. Ng, and T. G. F. Li, Extreme dark matter tests with extreme mass ratio inspirals, Phys. Rev. D 102
Original
1906
Earlier work this paper cites.
J. Jiang, A. C. Fabian, T. Dauser, L. Gallo, J. A. Garcia, E. Kara, M. L. Parker, J. A. Tomsick, D. J. Walton, and C. S. Reynolds, High Density Reflection Spectroscopy – II. The density of the inner black hole accretion disc in AGN, Mon. Not. Roy. Astron. Soc. 489
Original
1908
Earlier work this paper cites.
M. MacLeod and D. N. C. Lin, The Effect of Star-Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events, ApJ 889
Original
1909
Earlier work this paper cites.
O. Burke, J. R. Gair, and J. Simón, Transition from Inspiral to Plunge: A Complete Near-Extremal Trajectory and Associated Waveform, Phys. Rev. D 101
Original
1909
Earlier work this paper cites.
A. J. Dittmann and M. C. Miller, Star formation in accretion discs and SMBH growth, Mon. Not. Roy. Astron. Soc. 493
Original
1911
Earlier work this paper cites.
C. E. Scardoni, G. P. Rosotti, G. Lodato, and C. J. Clarke, Type II migration strikes back - an old paradigm for planet migration in discs, MNRAS 492
Original
1912
Earlier work this paper cites.
N. I. Shakura and R. A. Sunyaev, Black holes in binary systems. Observational appearance, Astron. Astrophys. 24
1973
Earlier work this paper cites.
A. P. Lightman and D. M. Eardley, Black Holes in Binary Systems: Instability of Disk Accretion, Astrophys. J. Lett. 187
1974
Earlier work this paper cites.
J. M. Bardeen and J. A. Petterson, The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes, Astrophys. J. Lett. 195
1975
Earlier work this paper cites.
N. I. Shakura and R. A. Sunyaev, A Theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars, Mon. Not. Roy. Astron. Soc. 175
1976
Earlier work this paper cites.
G. S. Bisnovatyi-Kogan and S. I. Blinnikov, Disk accretion onto a black hole at subcritical luminosity., A&A 59
1977
Earlier work this paper cites.
T. Piran, The role of viscosity and cooling mechanisms in the stability of accretion disks., ApJ 221
1978
Earlier work this paper cites.
P. Goldreich and S. Tremaine, Disk-satellite interactions., ApJ 241
1980
Earlier work this paper cites.
P. Sakimoto and F. Coroniti, Accretion disk models for qsos and active galactic nuclei - the role of magnetic viscosity, Astrophys. J. 247
1981
Earlier work this paper cites.
M. A. Abramowicz, B. Czerny, J. P. Lasota, and E. Szuszkiewicz, Slim accretion disks, Astrophys. J. 332
1988
Earlier work this paper cites.
D. Syer, C. J. Clarke, and M. J. Rees, Star-disc interactions near a massive black hole, MNRAS 250
1991
Earlier work this paper cites.
D. Syer and C. J. Clarke, Satellites in discs: regulating the accretion luminosity, MNRAS 277
1995
Earlier work this paper cites.
Y. Mino, M. Sasaki, and T. Tanaka, Gravitational radiation reaction to a particle motion, Phys. Rev. D 55
1997
Earlier work this paper cites.
T. C. Quinn and R. M. Wald, Axiomatic approach to electromagnetic and gravitational radiation reaction of particles in curved spacetime, Phys. Rev. D 56
1997
Earlier work this paper cites.
C. Cutler, Angular resolution of the LISA gravitational wave detector, Phys. Rev. D 57
1998
Earlier work this paper cites.
E. C. Ostriker, Dynamical friction in a gaseous medium, Astrophys. J. 513
1999
Earlier work this paper cites.
A. Ori and K. S. Thorne, Transition from inspiral to plunge for a compact body in a circular equatorial orbit around a massive, spinning black hole, Phys. Rev. D 62
2000
Earlier work this paper cites.
J. Goodman and R. R. Rafikov, Planetary torques as the viscosity of protoplanetary disks, Astrophys. J. 552
2001
Earlier work this paper cites.
J. Frank, A. King, and D. Raine, Accretion Power in Astrophysics , 3rd ed. (Cambridge University Press, 2002)
2002
Earlier work this paper cites.
H. Tanaka, T. Takeuchi, and W. R. Ward, Three-Dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration, ApJ 565
2002
Earlier work this paper cites.
B. J. Kavanagh, D. A. Nichols, G. Bertone, and D. Gaggero, Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform, Phys. Rev. D 102
Original
2002
Earlier work this paper cites.
Y. Levin, Formation of massive stars and black holes in selfgravitating AGN discs, and gravitational waves in LISA band (2003), arXiv:astro-ph/0307084
2003
Earlier work this paper cites.
L. Barack and C. Cutler, LISA capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy, Phys. Rev. D 69
2004
Earlier work this paper cites.
A. Maselli, N. Franchini, L. Gualtieri, and T. P. Sotiriou, Detecting scalar fields with Extreme Mass Ratio Inspirals, Phys. Rev. Lett. 125
Original
2004
Earlier work this paper cites.
A. Derdzinski, D. D’Orazio, P. Duffell, Z. Haiman, and A. MacFadyen, Evolution of gas disc–embedded intermediate mass ratio inspirals in the L I S A LISA band, Mon. Not. Roy. Astron. Soc. 501
Original
2005
Earlier work this paper cites.
K. Glampedakis and S. Babak, Mapping spacetimes with LISA: Inspiral of a test-body in a ‘quasi-Kerr’ field, Class. Quant. Grav. 23
2006
Earlier work this paper cites.
G. Fabj, S. S. Nasim, F. Caban, K. E. S. Ford, B. McKernan, and J. M. Bellovary, Aligning nuclear cluster orbits with an active galactic nucleus accretion disc, MNRAS 499
Original
2006
Earlier work this paper cites.
R. N. Lang and S. A. Hughes, Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession, Phys. Rev. D 74
2006
Earlier work this paper cites.
J. P. Gardner et al. , The James Webb Space Telescope, Space Sci. Rev. 123
2006
Earlier work this paper cites.
P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals, Class. Quant. Grav. 24
2007
Earlier work this paper cites.
E. Barausse, L. Rezzolla, D. Petroff, and M. Ansorg, Gravitational waves from Extreme Mass Ratio Inspirals in non-pure Kerr spacetimes, Phys. Rev. D 75
2007
Earlier work this paper cites.
P. Cresswell, G. Dirksen, W. Kley, and R. P. Nelson, On the evolution of eccentric and inclined protoplanets embedded in protoplanetary disks, A&A 473
Original
2007
Earlier work this paper cites.
L. Barack and C. Cutler, Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes, Phys. Rev. D 75
2007
Earlier work this paper cites.

Similar

T. Bogdanovic, C. S. Reynolds, and M. C. Miller, Alignment of the spins of supermassive black holes prior to merger, Astrophys. J. Lett. 661
2007
Cited alongside, same era.
E. Barausse, Relativistic dynamical friction in a collisional fluid, Mon. Not. Roy. Astron. Soc. 382
Original
2007
Cited alongside, same era.
Y. Levin, Starbursts near supermassive black holes: young stars in the Galactic Center, and gravitational waves in LISA band, Mon. Not. Roy. Astron. Soc. 374
2007
Cited alongside, same era.
P. F. Hopkins, G. T. Richards, and L. Hernquist, An Observational Determination of the Bolometric Quasar Luminosity Function, Astrophys. J. 654
2007
Cited alongside, same era.
L. Annulli, V. Cardoso, and R. Vicente, Stirred and shaken: Dynamical behavior of boson stars and dark matter cores, Phys. Lett. B 811
Original

Then

A. J. K. Chua, C. J. Moore, and J. R. Gair, Augmented kludge waveforms for detecting extreme-mass-ratio inspirals, Phys. Rev. D 96
Original
2017
Later among the works it cites.
K. Chamberlain and N. Yunes, Theoretical Physics Implications of Gravitational Wave Observation with Future Detectors, Phys. Rev. D 96
Original
2017
Later among the works it cites.
P. Amaro-Seoane, Relativistic dynamics and extreme mass ratio inspirals, Living Rev. Rel. 21
Original
2018
Later among the works it cites.
K. D. Kanagawa, H. Tanaka, and E. Szuszkiewicz, Radial Migration of Gap-opening Planets in Protoplanetary Disks. I. The Case of a Single Planet, ApJ 861
Original
2018
Later among the works it cites.
J. Aird, A. L. Coil, and A. Georgakakis, X-rays across the galaxy population – II. The distribution of AGN accretion rates as a function of stellar mass and redshift, Mon. Not. Roy. Astron. Soc. 474

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

2007

Cited alongside, same era.

J. D. Hunter, Matplotlib: A 2d graphics environment, Computing in Science & Engineering 9

2007

Cited alongside, same era.

E. Barausse and L. Rezzolla, The Influence of the hydrodynamic drag from an accretion torus on extreme mass-ratio inspirals, Phys. Rev. D 77

Original

2008

Cited alongside, same era.

A. J. K. Chua, M. L. Katz, N. Warburton, and S. A. Hughes, Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis, Phys. Rev. Lett. 126

Original

2008

Cited alongside, same era.

J. Casoli and F. S. Masset, On the Horseshoe Drag of a Low-Mass Planet. I. Migration in Isothermal Disks, ApJ 703

Original

2009

Cited alongside, same era.

S. J. Paardekooper and J. C. B. Papaloizou, On corotation torques, horseshoe drag and the possibility of sustained stalled or outward protoplanetary migration, MNRAS 394

Original

2009

Cited alongside, same era.

A. Perego, M. Dotti, M. Colpi, and M. Volonteri, Mass and spin coevolution during the alignment of a black hole in a warped accretion disc, Mon. Not. Roy. Astron. Soc. 399

Original

2009

Cited alongside, same era.

N. Yunes and F. Pretorius, Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework, Phys. Rev. D 80

Original

2009

Cited alongside, same era.

Original

2018