The Astrophysical Journal (Jan 2025)
Irregularly Sampled Time Series Interpolation for Detailed Binary Evolution Simulations
- Philipp M. Srivastava,
- Ugur Demir,
- Aggelos Katsaggelos,
- Vicky Kalogera,
- Shamal Lalvani,
- Elizabeth Teng,
- Tassos Fragos,
- Jeff J. Andrews,
- Simone S. Bavera,
- Max Briel,
- Seth Gossage,
- Konstantinos Kovlakas,
- Matthias U. Kruckow,
- Camille Liotine,
- Kyle A. Rocha,
- Meng Sun,
- Zepei Xing,
- Emmanouil Zapartas
Affiliations
- Philipp M. Srivastava
- ORCiD
- Electrical and Computer Engineering, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA; Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA
- Ugur Demir
- ORCiD
- Electrical and Computer Engineering, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA; Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA
- Aggelos Katsaggelos
- ORCiD
- Electrical and Computer Engineering, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA; Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA
- Vicky Kalogera
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA; Department of Physics and Astronomy, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA
- Shamal Lalvani
- ORCiD
- Electrical and Computer Engineering, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA
- Elizabeth Teng
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA; Department of Physics and Astronomy, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA
- Tassos Fragos
- ORCiD
- Département d’Astronomie, Université de Genève , Chemin Pegasi 51, CH-1290 Versoix, Switzerland; Gravitational Wave Science Center (GWSC), Université de Genève , CH1211 Geneva, Switzerland
- Jeff J. Andrews
- ORCiD
- Department of Physics, University of Florida , 2001 Museum Road, Gainesville, FL 32611, USA; Institute for Fundamental Theory , 2001 Museum Road, Gainesville, FL 32611, USA
- Simone S. Bavera
- ORCiD
- Département d’Astronomie, Université de Genève , Chemin Pegasi 51, CH-1290 Versoix, Switzerland; Gravitational Wave Science Center (GWSC), Université de Genève , CH1211 Geneva, Switzerland
- Max Briel
- ORCiD
- Département d’Astronomie, Université de Genève , Chemin Pegasi 51, CH-1290 Versoix, Switzerland; Gravitational Wave Science Center (GWSC), Université de Genève , CH1211 Geneva, Switzerland
- Seth Gossage
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA
- Konstantinos Kovlakas
- ORCiD
- Institute of Space Sciences (ICE, CSIC) , Campus UAB, Carrer de Magrans, 08193 Barcelona, Spain; Institut d’Estudis Espacials de Catalunya (IEEC) , Edifici RDIT, Campus UPC, 08860 Castelldefels (Barcelona), Spain
- Matthias U. Kruckow
- ORCiD
- Département d’Astronomie, Université de Genève , Chemin Pegasi 51, CH-1290 Versoix, Switzerland; Gravitational Wave Science Center (GWSC), Université de Genève , CH1211 Geneva, Switzerland
- Camille Liotine
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; Department of Physics and Astronomy, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA
- Kyle A. Rocha
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA; NSF-Simons AI Institute for the Sky (SkAI) , 172 E. Chestnut Street, Chicago, IL 60611, USA; Department of Physics and Astronomy, Northwestern University , 2145 Sheridan Road, Evanston, IL 60208, USA
- Meng Sun
- ORCiD
- Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University , 1800 Sherman Avenue, Evanston, IL 60201, USA
- Zepei Xing
- ORCiD
- Département d’Astronomie, Université de Genève , Chemin Pegasi 51, CH-1290 Versoix, Switzerland; Gravitational Wave Science Center (GWSC), Université de Genève , CH1211 Geneva, Switzerland
- Emmanouil Zapartas
- ORCiD
- Institute of Astrophysics, Foundation for Research and Technology-Hellas , GR-71110 Heraklion, Greece
- DOI
- https://doi.org/10.3847/1538-4357/adbe6b
- Journal volume & issue
-
Vol. 984,
no. 2
p. 154
Abstract
Modeling of large populations of binary stellar systems is an integral part of many areas of astrophysics, from radio pulsars and supernovae to X-ray binaries, gamma-ray bursts, and gravitational-wave mergers. Binary population synthesis codes that employ self-consistently the most advanced physics treatment available for stellar interiors and their evolution and are at the same time computationally tractable have started to emerge only recently. One element that is still missing from these codes is the ability to generate the complete time evolution of binaries with arbitrary initial conditions using precomputed three-dimensional grids of binary sequences. Here, we present a highly interpretable method, from binary evolution track interpolation. Our method implements simulation generation from irregularly sampled time series. Our results indicate that this method is appropriate for applications within binary population synthesis and computational astrophysics with time-dependent simulations in general. Furthermore, we point out and offer solutions to the difficulty surrounding evaluating the performance of signals exhibiting extreme morphologies akin to discontinuities.
Keywords