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Rev. Lett."],"accepted":{"date-parts":[[2026,6,10]]},"abstract":"<jats:p>\n                    Extending the sensitivity of terrestrial gravitational-wave detectors below 20\u00a0Hz is a long-standing challenge, limited by ground motion and inertial sensing noise. In this Letter, we demonstrate ultra-high-vacuum compatible inertial isolation and position sensing technologies that achieve active platform stabilization down to 10\u00a0mHz. Our laser position sensors reach a\n                    <a:math xmlns:a=\"http:\/\/www.w3.org\/1998\/Math\/MathML\" display=\"inline\">\n                      <a:mrow>\n                        <a:mi>sub<\/a:mi>\n                        <a:mtext>\u2212<\/a:mtext>\n                        <a:mi>pm<\/a:mi>\n                        <a:mo>\/<\/a:mo>\n                        <a:msqrt>\n                          <a:mrow>\n                            <a:mi>Hz<\/a:mi>\n                          <\/a:mrow>\n                        <\/a:msqrt>\n                      <\/a:mrow>\n                    <\/a:math>\n                    sensitivity above 10\u00a0mHz, independent of the input light polarization, representing a 100-fold improvement over the current LIGO position sensors. In addition, our inertial sensors provide at least a factor of 5 improvement in low-frequency sensitivity compared to state-of-the-art commercial seismometers. We integrate these technologies into a LIGO-like interferometer model and predict a low-frequency sensitivity improvement of up to an order of magnitude at 10\u00a0Hz, with enhanced linearity and calibration stability. This extension increases the detection horizon for intermediate-mass black hole binaries of mass\n                    <c:math xmlns:c=\"http:\/\/www.w3.org\/1998\/Math\/MathML\" display=\"inline\">\n                      <c:mrow>\n                        <c:msup>\n                          <c:mrow>\n                            <c:mn>10<\/c:mn>\n                          <\/c:mrow>\n                          <c:mrow>\n                            <c:mn>3<\/c:mn>\n                          <\/c:mrow>\n                        <\/c:msup>\n                        <c:msub>\n                          <c:mrow>\n                            <c:mi>M<\/c:mi>\n                          <\/c:mrow>\n                          <c:mrow>\n                            <c:mo stretchy=\"false\">\u2299<\/c:mo>\n                          <\/c:mrow>\n                        <\/c:msub>\n                      <\/c:mrow>\n                    <\/c:math>\n                    by a factor of 3 and increases the SNR for all lower mass binaries. Our results provide the first experimental demonstration of a practical pathway to sub-10\u00a0Hz operation of terrestrial gravitational-wave detectors and establish key technologies for next-generation observatories such as Cosmic Explorer and Einstein Telescope.\n                  <\/jats:p>","DOI":"10.1103\/65gz-dcjz","type":"journal-article","created":{"date-parts":[[2026,6,10]],"date-time":"2026-06-10T14:01:27Z","timestamp":1781100087000},"update-policy":"https:\/\/doi.org\/10.1103\/crossmark-policy","source":"Crossref","is-referenced-by-count":0,"title":["Extending Ground-Based Gravitational-Wave Sensitivity to 5\u00a0Hz"],"prefix":"10.1103","volume":"137","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-3240-6000","authenticated-orcid":true,"given":"Amit Singh","family":"Ubhi","sequence":"first","affiliation":[{"id":[{"id":"https:\/\/ror.org\/03angcq70","id-type":"ROR","asserted-by":"publisher"}],"name":"University of 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