50-km Fiber Interferometer for Testing Gravitational Signatures in Quantum Interference
Quantum mechanics and general relativity are the foundational pillars of modern physics, yet experimental tests that combine the two frameworks remain rare. Measuring optical phase shifts of massless photons in a gravitational potential provides a unique quantum platform to probe gravity beyond Newtonian descriptions, but laboratory-based interferometers have not yet reached the sensitivity needed to access this regime. Here, we report the realization of a 50-km table-top Mach-Zehnder fiber interferometer operating at the single-photon level, achieving a phase sensitivity of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:mrow> <a:mn>4.42</a:mn> <a:mo>×</a:mo> <a:msup> <a:mn>10</a:mn> <a:mrow> <a:mo>−</a:mo> <a:mn>6</a:mn> </a:mrow> </a:msup> <a:mtext> </a:mtext> <a:mtext> </a:mtext> <a:mi>rad</a:mi> </a:mrow> <a:mtext> </a:mtext> <a:mtext> </a:mtext> <a:mi>rms</a:mi> </a:math> within the frequency range of 0.01–5 Hz. We demonstrate that this sensitivity is sufficient to resolve a phase-shift signal of <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mrow> <c:mn>6.18</c:mn> <c:mo stretchy="false">(</c:mo> <c:mn>44</c:mn> <c:mo stretchy="false">)</c:mo> <c:mo>×</c:mo> <c:msup> <c:mn>10</c:mn> <c:mrow> <c:mo>−</c:mo> <c:mn>5</c:mn> </c:mrow> </c:msup> <c:mtext> </c:mtext> <c:mtext> </c:mtext> <c:mi>rad</c:mi> </c:mrow> <c:mtext> </c:mtext> <c:mtext> </c:mtext> <c:mi>rms</c:mi> </c:math> at 0.1 Hz, associated with a modulated gravity-induced signal. Our results establish a milestone for quantum sensing with large-scale optical interferometry, demonstrating the capability to detect gravitational redshifts in a local laboratory, thereby paving the way for testing quantum phenomena within general relativistic frameworks.
Authors
- Peter Barrow (ORCID: https://orcid.org/0000-0002-1620-7917)
- N. Mavalvala
- E. Polini (ORCID: https://orcid.org/0000-0003-4059-0765)
- Thomas Mieling (ORCID: https://orcid.org/0000-0002-6905-0183)
- Haocun Yu (ORCID: https://orcid.org/0000-0002-7597-098X)
- Piotr T. Chruściel (ORCID: https://orcid.org/0000-0001-8362-7340)
- Dorotea Macri (ORCID: https://orcid.org/0009-0006-0197-823X)
- Philip Walther (ORCID: https://orcid.org/0000-0002-4964-817X)
- E. Oelker (ORCID: https://orcid.org/0000-0002-3916-1595)
- Thomas Morling
- Christopher Hilweg (ORCID: https://orcid.org/0000-0003-0213-1234)
- Xinghui Yin
- Begüm Kabagöz
Institutions
- University of Vienna (AT)
- Austrian Academy of Sciences (AT)
- Center for Theoretical Physics (PL)
- Vienna Center for Quantum Science and Technology (AT)
- Massachusetts Institute of Technology (US)
- Polish Academy of Sciences (PL)
Publication Details
- Journal
- Physical Review Letters
- Published
- 2026-02-18
- DOI
- https://doi.org/10.1103/yvlk-t1j9
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00