activity
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

collaborators

32 papers

astro-ph.SR2025

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems

Abhishek Chattaraj, Jeff J. Andrews, Simone S. Bavera +14

With over two dozen detections in the Milky Way, double neutron stars (DNSs) provide a unique window into massive binary evolution. We use the POSYDON binary population synthesis c…

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.SR2024

Mass Transfer in Eccentric Orbits with Self-consistent Stellar Evolution

Kyle Akira Rocha, Rachel Hur, Vicky Kalogera +12

We investigate Roche lobe overflow mass transfer (MT) in eccentric binary systems between stars and compact objects (COs), modeling the coupled evolution of both the star and the o…

astro-ph.SR2024

Irregularly Sampled Time Series Interpolation for Detailed Binary Evolution Simulations

Philipp M. Srivastava, Ugur Demir, Aggelos Katsaggelos +14

Modeling of large populations of binary stellar systems is an intergral part of a many areas of astrophysics, from radio pulsars and supernovae to X-ray binaries, gamma-ray bursts,…

astro-ph.GA2024★ 4 cited

POSYDON Version 2: Population Synthesis with Detailed Binary-Evolution Simulations across a Cosmological Range of Metallicities

Jeff J. Andrews, Simone S. Bavera, Max Briel +21

Whether considering rare astrophysical events on cosmological scales or unresolved stellar populations, accurate models must account for the integrated contribution from the entire…

astro-ph.SR2024★ 15 cited

The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars

Matthias U. Kruckow, Jeff J. Andrews, Tassos Fragos +10

Context. The black holes discovered using Gaia, especially Gaia BH1 and BH2, have low mass companions of solar-like metallicity in wide orbits. For standard isolated binary evoluti…

astro-ph.SR2024★ 23 cited

The effect of mass loss in models of red supergiants in the Small Magellanic Cloud

E. Zapartas, S. de Wit, K. Antoniadis +16

The rate and mechanism of mass loss of red supergiants (RSGs) remain poorly understood, especially at low metallicities. Motivated by the new empirical prescription by Yang et al.…

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.SR2024★ 3 cited

Emulators for stellar profiles in binary population modeling

Elizabeth Teng, Ugur Demir, Zoheyr Doctor +14

Knowledge about the internal physical structure of stars is crucial to understanding their evolution. The novel binary population synthesis code POSYDON includes a module for inter…

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.SR2022★ 9 cited

Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations

Kyle Akira Rocha, Jeff J. Andrews, Christopher P. L. Berry +13

Binary stars undergo a variety of interactions and evolutionary phases, critical for predicting and explaining observed properties. Binary population synthesis with full stellar-st…

gr-qc2022★ 6 cited

Astrophysics with the Laser Interferometer Space Antenna

Pau Amaro Seoane, Jeff Andrews, Manuel Arca Sedda +156

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many…

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.SR2022★ 151 cited

POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations

Tassos Fragos, Jeff J. Andrews, Simone S. Bavera +22

Most massive stars are members of a binary or a higher-order stellar systems, where the presence of a binary companion can decisively alter their evolution via binary interactions.…