Search Results - "Endlich, S"

On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening by Leigh, N W C, Geller, A M, McKernan, B, Ford, K E S, Mac Low, M-M, Bellovary, J, Haiman, Z, Lyra, W, Samsing, J, O'Dowd, M, Kocsis, B, Endlich, S

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Constraining Stellar-mass Black Hole Mergers in AGN Disks Detectable with LIGO by McKernan, Barry, Saavik Ford, K. E., Bellovary, J., Leigh, N. W. C., Haiman, Z., Kocsis, B., Lyra, W., Mac Low, M.-M., Metzger, B., O'Dowd, M., Endlich, S., Rosen, D. J.

“…Black hole (BH) mergers detectable with the Laser Interferometer Gravitational-wave Observatory (LIGO) can occur in active galactic nucleus (AGN) disks. Here…”
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The effect of railway wheel wear on reprofiling and service life by Pires, A.C., Pacheco, L.A., Dalvi, I.L., Endlich, C.S., Queiroz, J.C., Antoniolli, F.A., Santos, G.F.M.

“…The aim of this study is to analyze how wheel wear affects the wheel reprofiling and service life and evaluate if these aspects can be improved by a new…”
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Influence of wheel tread wear on Rolling Contact Fatigue and on the dynamics of railway vehicles by Silva e Silva, J.V.R., Antoniolli, F.A., Endlich, C.S., Pires, A.C., Scandian, C., dos Santos, G.F.M.

“…This paper evaluates the influence of railway tread wear on the occurrence of Rolling Contact Fatigue (RCF) as well as other dynamic parameters of the railway…”
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On stellar-mass black hole mergers in AGN disks detectable with LIGO by McKernan, B, Ford, K. E. S, Bellovary, J, Leigh, N. W. C, Haiman, Z, Kocsis, B, Lyra, W, MacLow, M. -M, Metzger, B, O'Dowd, M, Endlich, S, Rosen, D. J

“…2018ApJ...866...66M Black hole mergers detectable with LIGO can occur in active galactic nucleus (AGN) disks. Here we parameterize the merger rates, the mass…”
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On the rate of black hole binary mergers in galactic nuclei due to dynamical hardening by Leigh, Nathan W. C, Geller, Aaron M, McKernan, B, Ford, K. E. S, Mac Low, M. -M, Bellovary, J, Haiman, Z, Lyra, W, Samsing, J, O'Dowd, M, Kocsis, B, Endlich, S

“…We assess the contribution of dynamical hardening by direct three-body scattering interactions to the rate of stellar-mass black hole binary (BHB) mergers in…”
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