Built on

G. P. Centers et al
Original
1905
Earlier work this paper cites.
Y. Himemoto and A. Taruya, “Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
J. I. Read, “The Local Dark Matter Density,” J. Phys. G
Original
1938
Earlier work this paper cites.
Springer New York, 1988
S. A. Kassam, Signal Detection in Non-Gaussian Noise · 1988
Earlier work this paper cites.
V. B. Braginsky, N. S. Kardashev, A. G. Polnarev, and I. D. Novikov, “Propagation of electromagnetic radiation in a random field of gravitational waves and space radio interferometry.,” Nuovo Cimento B Serie
1990
Earlier work this paper cites.
N. Christensen, “Measuring the stochastic gravitational radiation background with laser interferometric antennas,” Phys. Rev. D
1992
Earlier work this paper cites.
T. Pyne, C. R. Gwinn, M. Birkinshaw, T. M. Eubanks, and D. N. Matsakis, “Gravitational Radiation and Very Long Baseline Interferometry,” ApJ 465
1996
Earlier work this paper cites.
C. R. Gwinn, T. M. Eubanks, T. Pyne, M. Birkinshaw, and D. N. Matsakis, “Quasar proper motions and low frequency gravitational waves,” Astrophys. J
1997
Earlier work this paper cites.
B. Allen and J. D. Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D
1999
Earlier work this paper cites.
C. Mondino, A.-M. Taki, K. Van Tilburg, and N. Weiner, “First Results on Dark Matter Substructure from Astrometric Weak Lensing,” Phys. Rev. Lett
Original
2002
Earlier work this paper cites.
S. Mishra-Sharma, K. Van Tilburg, and N. Weiner, “Power of halometry,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
P. M. Meyers, K. Martinovic, N. Christensen, and M. Sakellariadou, “Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
S. L. Adler, “Placing direct limits on the mass of earth-bound dark matter,” J. Phys. A
Original
2008
Earlier work this paper cites.
M. Anholm, S. Ballmer, J. D. E. Creighton, L. R. Price, and X. Siemens, “Optimal strategies for gravitational wave stochastic background searches in pulsar timing data,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
P. Charlot, C. S. Jacobs, et al
Original
2010
Earlier work this paper cites.
Y. Wang, K. Pardo, T.-C. Chang, and O. Doré, “Gravitational Wave Detection with Photometric Surveys,” Phys. Rev. D
Original
2010
Earlier work this paper cites.
L. G. Book and E. E. Flanagan, “Astrometric Effects of a Stochastic Gravitational Wave Background,” Phys. Rev. D
Original
2011
Earlier work this paper cites.
N. Dalal, J. Bovy, L. Hui, and X. Li, “Don’t cross the streams: caustics from Fuzzy Dark Matter,” JCAP
Original
2011
Earlier work this paper cites.
O. Titov, S. B. Lambert, and A. M. Gontier, “VLBI measurement of the secular aberration drift,” Astron. Astrophys
Original
2011
Earlier work this paper cites.
F. Li, A. L. Erickcek, and N. M. Law, “A new probe of the small-scale primordial power spectrum: astrometric microlensing by ultracompact minihalos,” Phys. Rev. D
Original
2012
Earlier work this paper cites.

Similar

Gaia Collaboration, S. A. Klioner, et al
Original
2012
Cited alongside, same era.
P. F. de Salas and A. Widmark, “Dark matter local density determination: recent observations and future prospects,” Rept. Prog. Phys
Original
2012
Cited alongside, same era.
E. Thrane, N. Christensen, and R. Schofield, “Correlated magnetic noise in global networks of gravitational-wave interferometers: observations and implications,” Phys. Rev. D
Original
2013
Cited alongside, same era.
N. P. Pitjev and E. V. Pitjeva, “Constraints on dark matter in the solar system,” Astron. Lett
Original
2013
Cited alongside, same era.
H.-Y. Schive, T. Chiueh, and T. Broadhurst, “Cosmic Structure as the Quantum Interference of a Coherent Dark Wave,” Nature Phys

Then

D. J. E. Marsh and J. C. Niemeyer, “Strong Constraints on Fuzzy Dark Matter from Ultrafaint Dwarf Galaxy Eridanus II,” Phys. Rev. Lett
Original
2019
Later among the works it cites.
M. T. Penny, B. S. Gaudi, E. Kerins, N. J. Rattenbury, S. Mao, A. C. Robin, and S. Calchi Novati, “Predictions of the WFIRST Microlensing Survey. I. Bound Planet Detection Rates,” ApJS 241
Original
2019
Later among the works it cites.
WFIRST Astrometry Working Group, R. E. Sanderson, et al
Original
2019
Later among the works it cites.
S. T. Hodgkin, D. L. Harrison, et al
Original
2021
Later among the works it cites.
Y. Wang, K. Pardo, T.-C. Chang, and O. Doré, “Constraining the stochastic gravitational wave background with photometric surveys,” Phys. Rev. D

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2024

Astrometric Search for Ultralight Dark Matter

Kim, Hyungjin

Understand

Precision astrometry offers a way to probe new physics.

By measuring the angular position of light sources at unprecedented precision, astrometry could probe minuscule fluctuations of underlying spacetime.
This work explores the possibility of probing ultralight dark matter candidates using precision astrometry.
Through the coherent and stochastic density fluctuations over the scale of its wavelength, ultralight dark matter perturbs the propagation of light and the geodesics of the observer and source, leading to unique time-dependent signatures in the angular position of background light sources.

Built on

G. P. Centers et al
Original
1905
Earlier work this paper cites.
Y. Himemoto and A. Taruya, “Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
J. I. Read, “The Local Dark Matter Density,” J. Phys. G
Original
1938
Earlier work this paper cites.
Springer New York, 1988
S. A. Kassam, Signal Detection in Non-Gaussian Noise · 1988
Earlier work this paper cites.
V. B. Braginsky, N. S. Kardashev, A. G. Polnarev, and I. D. Novikov, “Propagation of electromagnetic radiation in a random field of gravitational waves and space radio interferometry.,” Nuovo Cimento B Serie
1990
Earlier work this paper cites.
N. Christensen, “Measuring the stochastic gravitational radiation background with laser interferometric antennas,” Phys. Rev. D
1992
Earlier work this paper cites.
T. Pyne, C. R. Gwinn, M. Birkinshaw, T. M. Eubanks, and D. N. Matsakis, “Gravitational Radiation and Very Long Baseline Interferometry,” ApJ 465
1996
Earlier work this paper cites.
C. R. Gwinn, T. M. Eubanks, T. Pyne, M. Birkinshaw, and D. N. Matsakis, “Quasar proper motions and low frequency gravitational waves,” Astrophys. J
1997
Earlier work this paper cites.
B. Allen and J. D. Romano, “Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities,” Phys. Rev. D
1999
Earlier work this paper cites.
C. Mondino, A.-M. Taki, K. Van Tilburg, and N. Weiner, “First Results on Dark Matter Substructure from Astrometric Weak Lensing,” Phys. Rev. Lett
Original
2002
Earlier work this paper cites.
S. Mishra-Sharma, K. Van Tilburg, and N. Weiner, “Power of halometry,” Phys. Rev. D
Original
2003
Earlier work this paper cites.
P. M. Meyers, K. Martinovic, N. Christensen, and M. Sakellariadou, “Detecting a stochastic gravitational-wave background in the presence of correlated magnetic noise,” Phys. Rev. D
Original
2008
Earlier work this paper cites.
S. L. Adler, “Placing direct limits on the mass of earth-bound dark matter,” J. Phys. A
Original
2008
Earlier work this paper cites.
M. Anholm, S. Ballmer, J. D. E. Creighton, L. R. Price, and X. Siemens, “Optimal strategies for gravitational wave stochastic background searches in pulsar timing data,” Phys. Rev. D
Original
2009
Earlier work this paper cites.
P. Charlot, C. S. Jacobs, et al
Original
2010
Earlier work this paper cites.
Y. Wang, K. Pardo, T.-C. Chang, and O. Doré, “Gravitational Wave Detection with Photometric Surveys,” Phys. Rev. D
Original
2010
Earlier work this paper cites.
L. G. Book and E. E. Flanagan, “Astrometric Effects of a Stochastic Gravitational Wave Background,” Phys. Rev. D
Original
2011
Earlier work this paper cites.
N. Dalal, J. Bovy, L. Hui, and X. Li, “Don’t cross the streams: caustics from Fuzzy Dark Matter,” JCAP
Original
2011
Earlier work this paper cites.
O. Titov, S. B. Lambert, and A. M. Gontier, “VLBI measurement of the secular aberration drift,” Astron. Astrophys
Original
2011
Earlier work this paper cites.
F. Li, A. L. Erickcek, and N. M. Law, “A new probe of the small-scale primordial power spectrum: astrometric microlensing by ultracompact minihalos,” Phys. Rev. D
Original
2012
Earlier work this paper cites.

Similar

Gaia Collaboration, S. A. Klioner, et al
Original
2012
Cited alongside, same era.
P. F. de Salas and A. Widmark, “Dark matter local density determination: recent observations and future prospects,” Rept. Prog. Phys
Original
2012
Cited alongside, same era.
E. Thrane, N. Christensen, and R. Schofield, “Correlated magnetic noise in global networks of gravitational-wave interferometers: observations and implications,” Phys. Rev. D
Original
2013
Cited alongside, same era.
N. P. Pitjev and E. V. Pitjeva, “Constraints on dark matter in the solar system,” Astron. Lett
Original
2013
Cited alongside, same era.
H.-Y. Schive, T. Chiueh, and T. Broadhurst, “Cosmic Structure as the Quantum Interference of a Coherent Dark Wave,” Nature Phys

Then

D. J. E. Marsh and J. C. Niemeyer, “Strong Constraints on Fuzzy Dark Matter from Ultrafaint Dwarf Galaxy Eridanus II,” Phys. Rev. Lett
Original
2019
Later among the works it cites.
M. T. Penny, B. S. Gaudi, E. Kerins, N. J. Rattenbury, S. Mao, A. C. Robin, and S. Calchi Novati, “Predictions of the WFIRST Microlensing Survey. I. Bound Planet Detection Rates,” ApJS 241
Original
2019
Later among the works it cites.
WFIRST Astrometry Working Group, R. E. Sanderson, et al
Original
2019
Later among the works it cites.
S. T. Hodgkin, D. L. Harrison, et al
Original
2021
Later among the works it cites.
Y. Wang, K. Pardo, T.-C. Chang, and O. Doré, “Constraining the stochastic gravitational wave background with photometric surveys,” Phys. Rev. D

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

Original

2014

Cited alongside, same era.

A. Khmelnitsky and V. Rubakov, “Pulsar timing signal from ultralight scalar dark matter,” JCAP

Original

2014

Cited alongside, same era.

E. Thrane, N. Christensen, R. M. S. Schofield, and A. Effler, “Correlated noise in networks of gravitational-wave detectors: subtraction and mitigation,” Phys. Rev. D

Original

2014

Cited alongside, same era.

A. Aoki and J. Soda, “Detecting ultralight axion dark matter wind with laser interferometers,” Int. J. Mod. Phys. D

Original

2016

Cited alongside, same era.

M. W. Coughlin et al

Original

2016

Cited alongside, same era.

A. Raccanelli, “Gravitational wave astronomy with radio galaxy surveys,” Mon. Not. Roy. Astron. Soc

Original

2017

Cited alongside, same era.

C. J. Moore, D. P. Mihaylov, A. Lasenby, and G. Gilmore, “Astrometric Search Method for Individually Resolvable Gravitational Wave Sources with Gaia,” Phys. Rev. Lett

Original

2017

Cited alongside, same era.

A. Bellini, S. Casertano, E. Nelan, and J. Kruk, “2MASS/Gaia as an Absolute Astrometric Reference Frame,” https://www.stsci.edu/files/live/sites/www/files/home/roman/_documents/WFIRST-STScI-TR1702.pdf , 2017

2017

Cited alongside, same era.

Original

2022

Later among the works it cites.

N. Dalal and A. Kravtsov, “Excluding fuzzy dark matter with sizes and stellar kinematics of ultrafaint dwarf galaxies,” Phys. Rev. D

Original

2022

Later among the works it cites.

H. Kim and A. Lenoci, “Gravitational focusing of wave dark matter,” Phys. Rev. D

Original

2022