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V. Vaskonen

As seen in: Nature, Physical Review B
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Articles by V. Vaskonen

A prototype differential atom interferometer for fundamental physics

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By D. Gareth Evans, L. Hawkins, D. N. Lee, B. Sauer, T. J. Walker, S. Dey, S. Hedges, M. Langlois, K. Bongs, J. Chen, Z. J. Eyler, C. Hsu, C. -Y. James Lu, J. F. Mitchell, J. Scheper, U. Schneider, X. Su, Y. L. Tang, S. Zhang, Y. Zhi, J. G. Carlton, J. A. Ellis, C. McCabe, D. Govardhan, V. Vaskonen, K. Peddlar Bridges, A. J. Carroll, J. L. Coleman, J. Tinsley, M. Craig Booth, N. Callaghan, K. L. Hughes, A. P. James, A. K. Lowe, J. W. Sander, D. Wood, K. Hussain, A. Marchant, Z. Pan, T. N. Valenzuela, M. van der Grinten, I. Wilmut, K. Clarke, C. F. A. Baynham, R. Hobson, O. Buchmüller, L. Iannizzotto Venezze, A. Josset, E. Pasatembou, M. R. Tarbutt, O. Ennis, U. Chauhan, A. Brzakalik, B. Stray, T. Hird, S. Lellouch, M. Holynski, B. Bostwick, V. Gibson, T. L. Harte, M. Karzazi, B. Millward, N. Mouelle, B. Panchumarthi, M. Zeuner, L. Badurina, A. Beniwal, D. Blas, G. Parish, T. Bowcock, G. Elertas, S. Hindley, C. Metelko, H. Throssell, E. Bentine, D. Bortoletto, C. Foot, C. Gómez-Monedero, T. Leese, J. March-Russell, J. Schelfhout, I. Shipsey, D. Weatherill, S. N. Balashov, M. G. Bason, H. Labiad, P. Majewski, D. Newbold, Z. Tam, T. C. Thornton, A. Vick
| Nature Verified
Abstract Gravitational waves and ultralight dark matter are among the most compelling frontiers in fundamental physics, motivating proposals for very-long-baseline atom interferometerssuch as AION1, MAGIS2, AICE3 and AEDGE4 that aim to detect at frequencies at which ground-based5 and space-borne6 laser interferometers lose sensitivity.
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Constraints on primordial black holes from LIGO-Virgo-KAGRA O3 events

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By M. Andrés-Carcasona, Dipartimento di Fisica, Sezione di Roma, V. Vaskonen
| Physical Review B
Primordial black holes (PBHs) can efficiently form black hole binaries in the early Universe. We update the resulting constraints on PBH abundance using data from the third observational run of LIGO-Virgo-KAGRA. To capture a wide range of PBH scenarios, we consider a variety of mass functions, including critical collapse in the QCD epoch and primordial non-Gaussianities.
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