Mass Transfer in Eccentric Orbits with Self-consistent Stellar Evolution Article Swipe
Kyle A. Rocha
,
Rachel Hur
,
V. Kalogera
,
Seth Gossage
,
Meng Sun
,
Z. Doctor
,
Jeff J. Andrews
,
Simone S. Bavera
,
Max M. Briel
,
Tassos Fragos
,
Konstantinos Kovlakas
,
Matthias U. Kruckow
,
Devina Misra
,
Zepei Xing
,
Emmanouil Zapartas
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb970
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/adb970
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 orbit due to eccentric MT (eMT) in a self-consistent framework. We implement the analytic expressions for secular rates of change of the orbital semimajor axis and eccentricity, assuming a delta function MT at periapse, in the binary stellar evolution code MESA . Two scenarios are examined: (1) a simplified model isolating the effects of eMT on stellar and orbital evolution, and (2) realistic binary configurations that include angular momentum exchange (e.g., tides, mass loss, spin–orbit coupling, and gravitational-wave (GW) radiation). Unlike the ad hoc approach of instant circularization that is often employed, explicit modeling of eMT reveals that a large fraction of binaries can remain eccentric post-MT. Even binaries that naturally circularize during eMT have different properties (donor mass and orbital size) compared to predictions from instant circularization, with some showing fundamentally different evolutionary outcomes (e.g., stable vs. unstable MT). We demonstrate that a binary’s initial mass ratio and eccentricity are predictive of whether it will remain eccentric or circularize after eMT. These findings underscore the importance of eMT in understanding CO-hosting binary populations, including X-ray binaries, GW sources, and other high-energy transients.
Related Topics
Concepts
Physics
Astrophysics
Astronomy
Stars
Stellar evolution
Stellar mass loss
Eccentric
Quantum mechanics
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/adb970
- OA Status
- gold
- Cited By
- 3
- References
- 150
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4409122967
All OpenAlex metadata
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https://openalex.org/W4409122967Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-4357/adb970Digital Object Identifier
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Mass Transfer in Eccentric Orbits with Self-consistent Stellar EvolutionWork title
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articleOpenAlex work type
- Language
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enPrimary language
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2025Year of publication
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2025-04-03Full publication date if available
- Authors
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Kyle A. Rocha, Rachel Hur, V. Kalogera, Seth Gossage, Meng Sun, Z. Doctor, Jeff J. Andrews, Simone S. Bavera, Max M. Briel, Tassos Fragos, Konstantinos Kovlakas, Matthias U. Kruckow, Devina Misra, Zepei Xing, Emmanouil ZapartasList of authors in order
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https://doi.org/10.3847/1538-4357/adb970Publisher landing page
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/adb970Direct OA link when available
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Physics, Astrophysics, Astronomy, Stars, Stellar evolution, Stellar mass loss, Eccentric, Quantum mechanicsTop concepts (fields/topics) attached by OpenAlex
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3Total citation count in OpenAlex
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2025: 3Per-year citation counts (last 5 years)
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150Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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