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20192025
most citedOne Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways

315 citations · 1.3k across the 31 of their papers we have counts for

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21 papers · 1 filter

astro-ph.HE2025★ 6 cited

A new long gamma-ray burst formation pathway at solar metallicity

M. M. Briel, T. Fragos, O. S. Salafia +11

Context. Long gamma-ray bursts (LGRBs) are generally observed in low-metallicity environments. However, 10 to 20 per cent of LGRBs at redshift are associated with near-solar…

astro-ph.HE2024★ 2 cited

Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries

Camille Liotine, Vicky Kalogera, Jeff J. Andrews +12

Binaries harboring a millisecond pulsar (MSP) and a black hole (BH) are a key observing target for current and upcoming pulsar surveys. We model the formation and evolution of such…

astro-ph.HE2024

Mass-gap Black Holes in Coalescing Neutron Star Black Hole Binaries

Zepei Xing, Vicky Kalogera, Tassos Fragos +10

The existence of a mass gap of between the heaviest neutron stars (NSs) and the lightest black holes (BHs), inferred from the BH mass distribution in low mass X-ra…

astro-ph.HE2024★ 7 cited

Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation

Zepei Xing, Tassos Fragos, Emmanouil Zapartas +12

The three dynamically confirmed wind-fed black hole high-mass X-ray binaries (BH-HMXBs) are suggested to all contain a highly spinning black hole (BH). However, based on the theori…

astro-ph.HE2023

Detecting the Undetected: Overcoming Biases in Gravitational-Wave Population Studies

Ryan Raikman, Simone Bavera, Tassos Fragos

In the flourishing field of gravitational-wave astronomy, accurately inferring binary black hole merger formation channels is paramount. The Bayesian hierarchical model selection a…

astro-ph.HE2023★ 3 cited

From ZAMS to Merger: Detailed Binary Evolution Models of Coalescing Neutron Star-Black Hole Systems at Solar Metallicity

Zepei Xing, Simone S. Bavera, Tassos Fragos +10

Neutron star black hole (NSBH) merger events bring us new opportunities to constrain theories of stellar and binary evolution, and understand the nature of compact objects. In…

astro-ph.HE2023★ 9 cited

Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations

Devina Misra, Konstantinos Kovlakas, Tassos Fragos +8

Ultra-luminous X-ray sources (ULXs) are sources observed to exceed the Eddington limit of a stellar-mass black hole (BH). A fraction of ULX sources show X-ray pulses which are evid…

astro-ph.HE2022★ 11 cited

Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3

Ying Qin, Yuan-Zhu Wang, Simone S. Bavera +10

The LIGO, Virgo, and KAGRA (LVK) collaboration has announced 90 coalescing binary black holes (BBHs) with to date, however, the origin of their formation cha…

astro-ph.HE2022★ 2 cited

The formation of merging black holes at solar metallicity

Simone S. Bavera, Tassos Fragos, Emmanouil Zapartas +11

The maximum mass of black holes formed in isolated binaries is determined by stellar winds and the interactions between the binary components. We consider for the first time fully…

astro-ph.HE2022★ 18 cited

A Black Hole Kicked At Birth: MAXI J1305-704

Chase Kimball, Sam Imperato, Vicky Kalogera +12

When a compact object is formed in a binary, any mass lost during core collapse will impart a kick on the binary's center of mass. Asymmetries in this mass loss or neutrino emissio…

astro-ph.HE2022★ 1 cited

Investigating the Lower Mass Gap with Low Mass X-ray Binary Population Synthesis

Jared C. Siegel, Ilia Kiato, Vicky Kalogera +14

Mass measurements from low-mass black hole X-ray binaries (LMXBs) and radio pulsars have been used to identify a gap between the most massive neutron stars (NSs) and the least mass…

astro-ph.HE2022★ 21 cited

X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations

Devina Misra, Konstantinos Kovlakas, Tassos Fragos +11

The ever-expanding observational sample of X-ray binaries (XRBs) makes them excellent laboratories for constraining binary evolution theory. Such constraints can be obtained by stu…

astro-ph.HE2022★ 35 cited

The correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it

Simone S. Bavera, Maya Fishbach, Michael Zevin +2

Understanding the origin of merging binary black holes is currently one of the most pressing quests in astrophysics. We show that if isolated binary evolution dominates the formati…

astro-ph.HE2022★ 66 cited

Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution

Michael Zevin, Simone S. Bavera

The LIGO and Virgo gravitational-wave detectors have uncovered binary black hole systems with definitively nonzero spins, as well as systems with significant spin residing in the m…

astro-ph.HE2021★ 41 cited

Probing the progenitors of spinning binary black-hole mergers with long gamma-ray bursts

Simone S. Bavera, Tassos Fragos, Emmanouil Zapartas +15

Long-duration gamma-ray bursts are thought to be associated with the core-collapse of massive, rapidly spinning stars and the formation of black holes. However, efficient angular m…

astro-ph.HE2021★ 42 cited

Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae

E. Zapartas, M. Renzo, T. Fragos +12

Stripped-envelope supernovae (Types IIb, Ib, and Ic) that show little or no hydrogen comprise roughly one-third of the observed explosions of massive stars. Their origin and the ev…

astro-ph.HE2021

Approximations to the spin of close Black-hole-Wolf-Rayet binaries

Simone S. Bavera, Michael Zevin, Tassos Fragos

Population synthesis studies of binary black-hole mergers often lack robust black-hole spin estimates as they cannot accurately follow tidal spin-up during the late black-hole-Wolf…

astro-ph.HE2020★ 35 cited

The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources

Jaime Román-Garza, Simone S. Bavera, Tassos Fragos +10

Recent detailed 1D core-collapse simulations have brought new insights on the final fate of massive stars, which are in contrast to commonly used parametric prescriptions. In this…

astro-ph.HE2020★ 315 cited

One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways

Michael Zevin, Simone S. Bavera, Christopher P. L. Berry +7

The second LIGO-Virgo catalog of gravitational wave transients has more than quadrupled the observational sample of binary black holes. We analyze this catalog using a suite of fiv…

astro-ph.HE2020★ 156 cited

The impact of mass-transfer physics on the observable properties of field binary black hole populations

Simone S. Bavera, Tassos Fragos, Michael Zevin +13

We study the impact of mass-transfer physics on the observable properties of binary black hole populations formed through isolated binary evolution. We investigate the impact of ma…

astro-ph.HE2019★ 254 cited

The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO

Simone S. Bavera, Tassos Fragos, Ying Qin +7

We study the formation of coalescing binary black holes via the evolution of isolated field binaries that go through the common envelope phase in order to obtain the combined distr…