Symmetries of spacetime infinitely far away from gravitational fields may hint at new laws of nature
Publications
Below are the publications with my direct contributions:
Goncharov, B., Thrane, E., Shannon, R. M., Harms, J., Bhat, N. D. R., Hobbs, G., Kerr, M., Manchester, R. N., Reardon, D. J., Russell, C. J., Zhu, X.-J., Zic, A., 2022. Consistency of the PPTA signal with a nanohertz gravitational wave background . arXiv preprint arXiv:2206.03766. Accepted in ApJ Letters.
Goncharov, B., Nitz, A.H. and Harms, J., 2022. Utilizing the null stream of Einstein Telescope. arXiv preprint arXiv:2204.08533.
Renzini, A.I., Goncharov, B., Jenkins, A.C. and Meyers, P.M., 2022. Stochastic Gravitational-Wave Backgrounds: Current Detection Efforts and Future Prospects. Galaxies, 10(1), p.34.
Ng, K.K., Chen, S., Goncharov, B., Dupletsa, U., Borhanian, S., Branchesi, M., Harms, J., Maggiore, M., Sathyaprakash, B.S. and Vitale, S., 2021. On the single-event-based identification of primordial black hole mergers at cosmological distances. arXiv preprint arXiv:2108.07276.
Goncharov, Boris, R. M. Shannon, D. J. Reardon, G. Hobbs, A. Zic, M. Bailes, M. Curyło et al. "On the Evidence for a Common-spectrum Process in the Search for the Nanohertz Gravitational-wave Background with the Parkes Pulsar Timing Array." The Astrophysical Journal Letters 917.2 (2021): L19.
Reardon, D.J., Shannon, R.M., Cameron, A.D., Goncharov, B., Hobbs, G.B., Middleton, H., Shamohammadi, M., Thyagarajan, N., Bailes, M., Bhat, N.D.R. and Dai, S., 2021. The Parkes pulsar timing array second data release: Timing analysis. Monthly Notices of the Royal Astronomical Society, 507(2), pp.2137-2153.
Goncharov, Boris, D. J. Reardon, R. M. Shannon, Xing-Jiang Zhu, Eric Thrane, M. Bailes, N. D. R. Bhat et al. "Identifying and mitigating noise sources in precision pulsar timing data sets." Monthly Notices of the Royal Astronomical Society 502, no. 1 (2021): 478-493.
Kerr, M., Reardon, D.J., Hobbs, G., Shannon, R.M., Manchester, R.N., Dai, S., Russell, C.J., Zhang, S.B., van Straten, W., Osłowski, S. and Parthasarathy, A., R. Spiewak, M. Bailes, N. D. R. Bhat, A. D. Cameron, W. A. Coles, J. Dempsey, X. Deng, B. Goncharov, et al. 32020. The Parkes Pulsar Timing Array Project: Second data release. arXiv preprint arXiv:2003.09780.
Goncharov, B., Zhu, X. J., & Thrane, E. (2019). Is there a spectral turnover in the spin noise of millisecond pulsars?. arXiv preprint arXiv:1910.05961. Monthly Notices of the Royal Astronomical Society (2020, accepted).
Ashton, G., Hübner, M., Lasky, P.D., Talbot, C., Ackley, K., Biscoveanu, S., Chu, Q., Divakarla, A., Easter, P.J., Goncharov, B., et al. Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy. The Astrophysical Journal Supplement Series 241.2 (2019): 27.
Goncharov, B., & Thrane, E. (2018). All-sky radiometer for narrowband gravitational waves using folded data. Physical Review D, 98(6), p. 064018.
Amelushkin, A.M., Bogomolov, V.V., Galkin, V.I., Goncharov, B.V., Gorbovskoy, E.S., Kornilov, V.G., Lipunov, V.M., Panasyuk, M.I., Petrov, V.L., Smoot, G.F. and Svertilov, S.I., 2013. BDRG and SHOK instruments for study of GRB prompt emission in Michaylo Lomonosov space mission. European Astronomical Society Publications Series, 61, pp.553-559.
Grossan, B., Smoot, G.F., Bogomolov, V.V., Svertilov, S.I., Vedenkin, N.N., Panasyuk, M., Goncharov, B., Rozhkov, G., Saleev, K., Grobovskoj, E. and Krasnov, A.S., 2013. Feasibility of a Small, Rapid Optical/IR Response, Next Generation Gamma-Ray Burst Mission. European Astronomical Society Publications Series, 61, pp.633-637.
Amelyushkin, A.M., Galkin, V.I., Goncharov, B.V., Gorbovskoy, E.S., Kornilov, V.G., Lipunov, V.M., Panasyuk, M.I., Petrov, V.L., Smoot, G.F., Svertilov, S.I. and Vedenkin, N.N., 2013. The BDRG and SHOK instruments for studying gamma-ray burst prompt emission onboard the Lomonosov spacecraft. Cosmic Research, 51(6), pp.434-438.All citations according to Google Scholar 61141, h-index 76 (collaboration papers included):
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Recent Work
Is the common-spectrum process observed with pulsar timing arrays a precursor to the detection?