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_citations.md

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## Citation Summary
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- **Total ADS citations**: 9667
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- **Total INSPIRE citations**: 10520
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- **Total MAX citations**: 10604
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- **Total ADS citations**: 9677
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- **Total INSPIRE citations**: 10532
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- **Total MAX citations**: 10616
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- **h-index**: 47
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## Paper list sorted by citation count
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| # | Author | Year | Title | ADS | INSPIRE | MAX |
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|---|--------|------|-------|-----|---------|-----|
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1409 | 1581 | 1581 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 836 | 924 | 924 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 730 | 680 | 730 |
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| **1** | Berti | 2015 | Testing general relativity with present and future astrophysical observations | 1410 | 1582 | 1582 |
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| **2** | Barack | 2019 | Black holes, gravitational waves and fundamental physics: a roadmap | 836 | 926 | 926 |
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| **3** | Amaro-Seoane | 2022 | Astrophysics with the Laser Interferometer Space Antenna | 731 | 681 | 731 |
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| **4** | Belczynski | 2020 | Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes | 455 | 471 | 471 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 426 | 442 | 442 |
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| **5** | Varma | 2019 | Surrogate models for precessing binary black hole simulations with unequal masses | 428 | 442 | 442 |
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| **6** | Barausse | 2020 | Prospects for fundamental physics with LISA | 389 | 439 | 439 |
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| **7** | Gerosa | 2017 | Are merging black holes born from stellar collapse or previous mergers? | 329 | 354 | 354 |
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| **8** | Arun | 2022 | New horizons for fundamental physics with LISA | 299 | 351 | 351 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 262 | 278 | 278 |
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| **8** | Arun | 2022 | New horizons for fundamental physics with LISA | 299 | 353 | 353 |
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| **9** | Gerosa | 2021 | Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures | 263 | 278 | 278 |
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| **10** | Gerosa | 2018 | Spin orientations of merging black holes formed from the evolution of stellar binaries | 214 | 235 | 235 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 169 | 169 |
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| **11** | Afshordi | 2025 | Waveform modelling for the Laser Interferometer Space Antenna | 144 | 171 | 171 |
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| **12** | Gerosa | 2015 | Multi-timescale analysis of phase transitions in precessing black-hole binaries | 138 | 161 | 161 |
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| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 142 | 159 | 159 |
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| **13** | Varma | 2019 | High-accuracy mass, spin, and recoil predictions of generic black-hole merger remnants | 143 | 159 | 159 |
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| **14** | Gerosa | 2013 | Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation | 143 | 158 | 158 |
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| **15** | Islam | 2021 | Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case | 127 | 138 | 138 |
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| **16** | Kesden | 2015 | Effective potentials and morphological transitions for binary black-hole spin precession | 115 | 137 | 137 |
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| **23** | Wysocki | 2018 | Explaining LIGO's observations via isolated binary evolution with natal kicks | 96 | 101 | 101 |
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| **24** | Gerosa | 2016 | PRECESSION: Dynamics of spinning black-hole binaries with python | 92 | 101 | 101 |
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| **25** | Vitale | 2017 | Impact of Bayesian priors on the characterization of binary black hole coalescences | 86 | 99 | 99 |
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| **26** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 96 | 96 |
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| **27** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 95 | 95 |
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| **26** | Romero-Shaw | 2023 | Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data | 82 | 96 | 96 |
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| **27** | Taylor | 2018 | Mining gravitational-wave catalogs to understand binary stellar evolution: a new hierarchical bayesian framework | 92 | 96 | 96 |
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| **28** | Baibhav | 2020 | The mass gap, the spin gap, and the origin of merging binary black holes | 79 | 91 | 91 |
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| **29** | O'Shaughnessy | 2017 | Inferences about supernova physics from gravitational-wave measurements: GW151226 spin misalignment as an indicator of strong black-hole natal kicks | 79 | 87 | 87 |
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| **30** | Gerosa | 2021 | A generalized precession parameter $$\chi_\mathrm{p}$$ to interpret gravitational-wave data | 67 | 78 | 78 |
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| **31** | Bouffanais | 2019 | Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data | 76 | 78 | 78 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 76 | 76 | 76 |
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| **32** | Korol | 2020 | Populations of double white dwarfs in Milky Way satellites and their detectability with LISA | 77 | 76 | 77 |
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| **33** | Horbatsch | 2015 | Tensor-multi-scalar theories: relativistic stars and 3+1 decomposition | 70 | 74 | 74 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 61 | 67 | 67 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 61 | 66 | 66 |
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| **34** | Klein | 2022 | The last three years: multiband gravitational-wave observations of stellar-mass binary black holes | 61 | 68 | 68 |
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| **35** | Gerosa | 2016 | Black-hole kicks as new gravitational-wave observables | 62 | 66 | 66 |
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| **36** | Buscicchio | 2021 | Bayesian parameter estimation of stellar-mass black-hole binaries with LISA | 55 | 64 | 64 |
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| **37** | Gupta | 2020 | Black holes in the low mass gap: Implications for gravitational wave observations | 58 | 63 | 63 |
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| **38** | Gerosa | 2018 | Black-hole kicks from numerical-relativity surrogate models | 56 | 62 | 62 |
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| **39** | Gerosa | 2015 | Precessional instability in binary black holes with aligned spins | 56 | 61 | 61 |
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| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 53 | 60 | 60 |
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| **40** | Gerosa | 2020 | Astrophysical implications of GW190412 as a remnant of a previous black-hole merger | 54 | 60 | 60 |
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| **41** | Gerosa | 2016 | Numerical simulations of stellar collapse in scalar-tensor theories of gravity | 52 | 60 | 60 |
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| **42** | Gerosa | 2014 | Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures | 47 | 57 | 57 |
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| **43** | Mould | 2022 | Deep learning and Bayesian inference of gravitational-wave populations: hierarchical black-hole mergers | 52 | 56 | 56 |
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| **52** | Trifiro' | 2016 | Distinguishing black-hole spin-orbit resonances by their gravitational wave signatures. II: Full parameter estimation | 34 | 42 | 42 |
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| **53** | Gerosa | 2020 | Gravitational-wave selection effects using neural-network classifiers | 37 | 41 | 41 |
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| **54** | Santini | 2023 | Black-hole mergers in disk-like environments could explain the observed $$q-\chi_\mathrm{eff}$$ correlation | 40 | 39 | 40 |
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| **55** | Lodato | 2013 | Black hole mergers: do gas discs lead to spin alignment? | 38 | 37 | 38 |
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| **55** | Lodato | 2013 | Black hole mergers: do gas discs lead to spin alignment? | 38 | 38 | 38 |
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| **56** | Rosca-Mead | 2020 | Core collapse in massive scalar-tensor gravity | 27 | 34 | 34 |
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| **57** | Gerosa | 2021 | High mass but low spin: an exclusion region to rule out hierarchical black-hole mergers as a mechanism to populate the pair-instability mass gap | 29 | 32 | 32 |
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| **58** | Gerosa | 2023 | Efficient multi-timescale dynamics of precessing black-hole binaries | 28 | 31 | 31 |
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| **66** | Rosca-Mead | 2020 | Structure of neutron stars in massive scalar-tensor gravity | 23 | 26 | 26 |
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| **67** | Pacilio | 2024 | Flexible mapping of ringdown amplitudes for nonprecessing binary black holes | 21 | 25 | 25 |
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| **68** | Boschini | 2025 | Orbital eccentricity in general relativity from catastrophe theory | 22 | 24 | 24 |
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| **69** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
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| **70** | Croon | 2025 | Can stellar physics explain GW231123? | 23 | 23 | 23 |
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| **71** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 22 | 23 | 23 |
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| **69** | Fumagalli | 2023 | Spin-eccentricity interplay in merging binary black holes | 22 | 24 | 24 |
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| **70** | Moore | 2021 | Population-informed priors in gravitational-wave astronomy | 24 | 23 | 24 |
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| **71** | Croon | 2025 | Can GW231123 have a stellar origin? | 23 | 23 | 23 |
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| **72** | Zhao | 2017 | Nutational resonances, transitional precession, and precession-averaged evolution in binary black-hole systems | 21 | 23 | 23 |
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| **73** | Gerosa | 2017 | On the equal-mass limit of precessing black-hole binaries | 19 | 23 | 23 |
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| **74** | Mould | 2020 | Endpoint of the up-down instability in precessing binary black holes | 18 | 22 | 22 |
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| **75** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 21 | 22 | 22 |
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| **75** | Sperhake | 2020 | Amplification of superkicks in black-hole binaries through orbital eccentricity | 22 | 22 | 22 |
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| **76** | Gerosa | 2019 | Wide nutation: binary black-hole spins repeatedly oscillating from full alignment to full anti-alignment | 20 | 22 | 22 |
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| **77** | Romero-Shaw | 2025 | GW200208_222617 as an eccentric black-hole binary merger: properties and astrophysical implications | 21 | 20 | 21 |
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| **78** | Mancarella | 2023 | Inferring, not just detecting: metrics for high-redshift sources observed with third-generation gravitational-wave detectors | 16 | 21 | 21 |
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*Last updated: 2026-01-27 01:01:15 UTC*

_group.md

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_publications.md

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Physical Review D, in press. <a href="https://arxiv.org/abs/2505.16795" style="color: inherit; text-decoration: none;">arXiv:2505.16795 [gr-qc]</a>.
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**107.**
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*Can stellar physics explain GW231123?*\
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D. Croon, J. Sakstein, **D. Gerosa**.\
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*Can GW231123 have a stellar origin?*\
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D. Croon, **D. Gerosa**, J. Sakstein.\
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Monthly Notices of the Royal Astronomical Society, in press. <a href="https://arxiv.org/abs/2508.10088" style="color: inherit; text-decoration: none;">arXiv:2508.10088 [astro-ph.HE]</a>.
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_talks.md

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parsepapers.tex

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{\prd, in press}. \href{https://arxiv.org/abs/2505.16795}{arXiv:2505.16795 [gr-qc].}
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\textbf{107.} & & \textit{Can stellar physics explain GW231123?}
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\textbf{107.} & & \textit{Can GW231123 have a stellar origin?}
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\newline{}
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D. Croon, J. Sakstein, \textbf{D. Gerosa}.
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D. Croon, \textbf{D. Gerosa}, J. Sakstein.
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{\mnras, in press}. \href{https://arxiv.org/abs/2508.10088}{arXiv:2508.10088 [astro-ph.HE].}
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