Zobrazeno 1 - 10
of 99
pro vyhledávání: '"Mihaylov, Deyan"'
Autor:
Saha, Samanta, Copi, Craig J., Starkman, Glenn D., Anselmi, Stefano, Duque, Javier Carrón, Barandiaran, Mikel Martin, Akrami, Yashar, Cornet-Gomez, Fernando, Jaffe, Andrew H., Kosowsky, Arthur, Mihaylov, Deyan P., Pereira, Thiago S., Samandar, Amirhossein, Tamosiunas, Andrius
Cosmic microwave background (CMB) temperature and polarization observations indicate that in the best-fit $\Lambda$ Cold Dark Matter model of the Universe, the local geometry is consistent with at most a small amount of positive or negative curvature
Externí odkaz:
http://arxiv.org/abs/2409.02226
Autor:
Samandar, Amirhossein, Duque, Javier Carrón, Copi, Craig J., Barandiaran, Mikel Martin, Mihaylov, Deyan P., Pereira, Thiago S., Starkman, Glenn D., Akrami, Yashar, Anselmi, Stefano, Cornet-Gomez, Fernando, Eskilt, Johannes R., Jaffe, Andrew H., Kosowsky, Arthur, Tamosiunas, Andrius
Publikováno v:
JCAP 11 (2024) 020
The standard cosmological model, which assumes statistical isotropy and parity invariance, predicts the absence of correlations between even-parity and odd-parity observables of the cosmic microwave background (CMB). Contrary to these predictions, la
Externí odkaz:
http://arxiv.org/abs/2407.09400
Autor:
Tamosiunas, Andrius, Cornet-Gomez, Fernando, Akrami, Yashar, Anselmi, Stefano, Duque, Javier Carrón, Copi, Craig J., Eskilt, Johannes R., Güngör, Özenç, Jaffe, Andrew H., Kosowsky, Arthur, Barandiaran, Mikel Martin, Mertens, James B., Mihaylov, Deyan P., Pereira, Thiago S., Saha, Samanta, Samandar, Amirhossein, Starkman, Glenn D., Taylor, Quinn, Vardanyan, Valeri
Publikováno v:
JCAP 09 (2024) 057
Non-trivial spatial topology of the Universe may give rise to potentially measurable signatures in the cosmic microwave background. We explore different machine learning approaches to classify harmonic-space realizations of the microwave background i
Externí odkaz:
http://arxiv.org/abs/2404.01236
Autor:
Taylor, Quinn, Starkman, Glenn D., Hinczewski, Michael, Mihaylov, Deyan P., Silk, Joseph, Pacheco, Jose de Freitas
The Hawking process results in a monotonic decrease of the black hole mass, but a biased random walk of the black hole angular momentum. We demonstrate that this stochastic process leads to a significant fraction of primordial black holes becoming ex
Externí odkaz:
http://arxiv.org/abs/2403.04054
Autor:
Eskilt, Johannes R., Akrami, Yashar, Anselmi, Stefano, Copi, Craig J., Jaffe, Andrew H., Kosowsky, Arthur, Mihaylov, Deyan P., Starkman, Glenn D., Tamosiunas, Andrius, Mertens, James B., Petersen, Pip, Saha, Samanta, Taylor, Quinn, Güngör, Özenç
Publikováno v:
JCAP 03 (2024) 036
If the Universe has non-trivial spatial topology, observables depend on both the parameters of the spatial manifold and the position and orientation of the observer. In infinite Euclidean space, most cosmological observables arise from the amplitudes
Externí odkaz:
http://arxiv.org/abs/2306.17112
Autor:
Mihaylov, Deyan P., Ossokine, Serguei, Buonanno, Alessandra, Estelles, Hector, Pompili, Lorenzo, Pürrer, Michael, Ramos-Buades, Antoni
We present pySEOBNR, a Python package for gravitational-wave (GW) modeling developed within the effective-one-body (EOB) formalism. The package contains an extensive framework to generate state-of-the-art inspiral-merger-ringdown waveform models for
Externí odkaz:
http://arxiv.org/abs/2303.18203
Autor:
Khalil, Mohammed, Buonanno, Alessandra, Estellés, Héctor, Mihaylov, Deyan P., Ossokine, Serguei, Pompili, Lorenzo, Ramos-Buades, Antoni
Waveform models are essential for gravitational-wave (GW) detection and parameter estimation of coalescing compact-object binaries. More accurate models are required for the increasing sensitivity of current and future GW detectors. The effective-one
Externí odkaz:
http://arxiv.org/abs/2303.18143
Autor:
Ramos-Buades, Antoni, Buonanno, Alessandra, Estellés, Héctor, Khalil, Mohammed, Mihaylov, Deyan P., Ossokine, Serguei, Pompili, Lorenzo, Shiferaw, Mahlet
Spin precession is one of the key physical effects that could unveil the origin of the compact binaries detected by ground- and space-based gravitational-wave (GW) detectors, and shed light on their possible formation channels. Efficiently and accura
Externí odkaz:
http://arxiv.org/abs/2303.18046
Autor:
Pompili, Lorenzo, Buonanno, Alessandra, Estellés, Héctor, Khalil, Mohammed, van de Meent, Maarten, Mihaylov, Deyan P., Ossokine, Serguei, Pürrer, Michael, Ramos-Buades, Antoni, Mehta, Ajit Kumar, Cotesta, Roberto, Marsat, Sylvain, Boyle, Michael, Kidder, Lawrence E., Pfeiffer, Harald P., Scheel, Mark A., Rüter, Hannes R., Vu, Nils, Dudi, Reetika, Ma, Sizheng, Mitman, Keefe, Melchor, Denyz, Thomas, Sierra, Sanchez, Jennifer
We present SEOBNRv5HM, a more accurate and faster inspiral-merger-ringdown gravitational waveform model for quasi-circular, spinning, nonprecessing binary black holes within the effective-one-body (EOB) formalism. Compared to its predecessor, SEOBNRv
Externí odkaz:
http://arxiv.org/abs/2303.18039
Autor:
van de Meent, Maarten, Buonanno, Alessandra, Mihaylov, Deyan P., Ossokine, Serguei, Pompili, Lorenzo, Warburton, Niels, Pound, Adam, Wardell, Barry, Durkan, Leanne, Miller, Jeremy
We leverage recent breakthrough calculations using second-order gravitational self-force (2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction force in effective-one-body~(EOB) waveform models. We achieve this by intr
Externí odkaz:
http://arxiv.org/abs/2303.18026