Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Leong, Samson H. W."'
Autor:
Bustillo, Juan Calderón, del Rio, Adrian, Sanchis-Gual, Nicolas, Chandra, Koustav, Leong, Samson H. W.
Precessing black-hole mergers can produce gravitational waves with net circular polarization, understood as an imbalance between right- and left-handed amplitudes. According to the Cosmological Principle, such emission must average to zero across all
Externí odkaz:
http://arxiv.org/abs/2402.09861
Observation of gravitational waves from inspiralling binary black holes has offered a unique opportunity to study the physical parameters of the component black holes. To infer these parameters, Bayesian methods are employed in conjunction with gener
Externí odkaz:
http://arxiv.org/abs/2309.01683
Publikováno v:
Phys. Rev. D 108, 124079 (2023)
Dense environments hosting compact binary mergers can leave an imprint on the gravitational-wave emission which, in turn, can be used to identify the characteristics of the environment. To demonstrate such scenario, we consider a simple setup of bina
Externí odkaz:
http://arxiv.org/abs/2308.03250
Autor:
Liu, Anna, Wong, Isaac C. F., Leong, Samson H. W., More, Anupreeta, Hannuksela, Otto A., Li, Tjonnie G. F.
Since the first detection of gravitational waves in 2015, gravitational-wave astronomy has emerged as a rapidly advancing field that holds great potential for studying the cosmos, from probing the properties of black holes to testing the limits of ou
Externí odkaz:
http://arxiv.org/abs/2302.09870
General relativity predicts that gravitational waves (GWs) carry linear momentum. Consequently, the remnant black hole of a black-hole merger can inherit a recoil velocity or ``kick'' of crucial implications in, e.g, black-hole formation scenarios. W
Externí odkaz:
http://arxiv.org/abs/2211.03465
Autor:
Sanchis-Gual, Nicolas, Bustillo, Juan Calderón, Herdeiro, Carlos, Radu, Eugen, Font, José A., Leong, Samson H. W., Torres-Forné, Alejandro
Publikováno v:
Phys. Rev. D 106, 124011 - Published 6 December 2022
We present a systematic study of the dynamics and gravitational-wave emission of head-on collisions of spinning vector boson stars, known as Proca stars. To this aim we build a catalogue of about 800 numerical-relativity simulations of such systems.
Externí odkaz:
http://arxiv.org/abs/2208.11717
Autor:
Bustillo, Juan Calderon, Sanchis-Gual, Nicolas, Leong, Samson H. W., Chandra, Koustav, Torres-Forne, Alejandro, Font, Jose A., Herdeiro, Carlos, Radu, Eugen, Wong, Isaac C. F., Li, T. G. F.
We present the first systematic search for exotic compact mergers in Advanced LIGO and Virgo events. We compare the short gravitational-wave signals GW190521, GW190426$\_$190642, GW200220$\_$061928 and the trigger 200114$\_$020818 (or S200114f) to a
Externí odkaz:
http://arxiv.org/abs/2206.02551
Autor:
Bustillo, Juan Calderon, Wong, Isaac C. F., Sanchis-Gual, Nicolas, Leong, Samson H. W., Torres-Forne, Alejandro, Chandra, Koustav, Font, Jose A., Herdeiro, Carlos, Radu, Eugen, Li, T. G. F.
Detection and parameter inference of gravitational-wave signals \ncor{from compact mergers} rely on the comparison of the incoming detector strain data $d(t)$ to waveform templates for the gravitational-wave strain $h(t)$ that ultimately rely on the
Externí odkaz:
http://arxiv.org/abs/2205.15029
Autor:
Bustillo, Juan Calderón, Leong, Samson H. W., Chandra, Koustav, McKernan, Barry, Ford, K. E. S.
We present an analysis that reconciles the gravitational-wave signal GW190521 observed by the Advanced LIGO and Advanced Virgo detectors with the electromagnetic flare ZTF19abanrhr observed by the Zwicky Transient Facility. We analyze GW190521 under
Externí odkaz:
http://arxiv.org/abs/2112.12481
Autor:
Bustillo, Juan Calderón, Sanchis-Gual, Nicolas, Torres-Forné, Alejandro, Font, José A., Vajpeyi, Avi, Smith, Rory, Herdeiro, Carlos, Radu, Eugen, Leong, Samson H. W.
Publikováno v:
Phys. Rev. Lett. 126, 081101 (2021)
Advanced LIGO-Virgo reported a short gravitational-wave signal (GW190521) interpreted as a quasi-circular merger of black holes, one populating the pair-instability supernova gap, forming a remnant black hole of $M_f\sim 142 M_\odot$ at a luminosity
Externí odkaz:
http://arxiv.org/abs/2009.05376