Two-photon amplitude interferometry for precision astrometry
Improved quantum sensing of photons from astronomical objects could provide high resolution observations in the optical benefiting numerous fields, including general relativity, dark matter studies, and cosmology. It has been recently proposed that stations in optical interferometers would not requi...
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Published in | The open journal of astrophysics Vol. 5; no. 1 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Maynooth Academic Publishing
01.11.2022
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Online Access | Get full text |
ISSN | 2565-6120 2565-6120 |
DOI | 10.21105/astro.2010.09100 |
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Abstract | Improved quantum sensing of photons from astronomical objects could provide high resolution observations in the optical benefiting numerous fields, including general relativity, dark matter studies, and cosmology. It has been recently proposed that stations in optical interferometers would not require a phase-stable optical link if instead sources of quantum-mechanically entangled pairs could be provided to them, potentially enabling hitherto prohibitively long baselines. A new refinement of this idea is developed, in which two photons from different sources are interfered at two separate and decoupled stations, requiring only a slow classical information link between them. We rigorously calculate the observables and contrast this new interferometric technique with the Hanbury Brown \& Twiss intensity interferometry. We argue this technique could allow robust high-precision measurements of the relative astrometry of the two sources. A basic calculation suggests that angular precision on the order of $10$ microarcseconds in the relative opening angle could be achieved in a single night's observation of two bright stars. |
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AbstractList | Improved quantum sensing of photons from astronomical objects could provide high resolution observations in the optical benefiting numerous fields, including general relativity, dark matter studies, and cosmology. It has been recently proposed that stations in optical interferometers would not require a phase-stable optical link if instead sources of quantum-mechanically entangled pairs could be provided to them, potentially enabling hitherto prohibitively long baselines. A new refinement of this idea is developed, in which two photons from different sources are interfered at two separate and decoupled stations, requiring only a slow classical information link between them. We rigorously calculate the observables and contrast this new interferometric technique with the Hanbury Brown \& Twiss intensity interferometry. We argue this technique could allow robust high-precision measurements of the relative astrometry of the two sources. A basic calculation suggests that angular precision on the order of $10$ microarcseconds in the relative opening angle could be achieved in a single night's observation of two bright stars. |
Author | Stankus, Paul Nomerotski, Andrei Vintskevich, Stephen Slosar, Anže |
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CitedBy_id | crossref_primary_10_1103_PhysRevD_109_123029 crossref_primary_10_1364_OE_486342 crossref_primary_10_1103_PhysRevA_107_032421 crossref_primary_10_1109_JSTQE_2025_3545414 crossref_primary_10_1103_PhysRevD_107_023015 crossref_primary_10_1103_PhysRevLett_131_210801 crossref_primary_10_1063_5_0226069 crossref_primary_10_1038_s41377_024_01684_y crossref_primary_10_1126_sciadv_adh1439 crossref_primary_10_1088_1748_0221_18_01_C01023 crossref_primary_10_1088_1748_0221_19_12_P12015 crossref_primary_10_1364_OE_543511 crossref_primary_10_1063_5_0168423 |
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