Integrating astrochemistry in hydrodynamics

Niels Bohr Institute

Integrating astrochemistry in hydrodynamics

Research output: Chapter in Book/Report/Conference proceeding › Book chapter › Research › peer-review

Standard

Integrating astrochemistry in hydrodynamics. / Haugbølle, Troels; Lupi, Alessandro; Ramsey, Jon.

Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations. Elsevier, 2024. p. 323-336.

Research output: Chapter in Book/Report/Conference proceeding › Book chapter › Research › peer-review

Harvard

Haugbølle, T, Lupi, A & Ramsey, J 2024, Integrating astrochemistry in hydrodynamics. in Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations. Elsevier, pp. 323-336. https://doi.org/10.1016/B978-0-32-391746-9.00022-5

APA

Haugbølle, T., Lupi, A., & Ramsey, J. (2024). Integrating astrochemistry in hydrodynamics. In Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations (pp. 323-336). Elsevier. https://doi.org/10.1016/B978-0-32-391746-9.00022-5

Vancouver

Haugbølle T, Lupi A, Ramsey J. Integrating astrochemistry in hydrodynamics. In Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations. Elsevier. 2024. p. 323-336 https://doi.org/10.1016/B978-0-32-391746-9.00022-5

Author

Haugbølle, Troels ; Lupi, Alessandro ; Ramsey, Jon. / Integrating astrochemistry in hydrodynamics. Astrochemical Modeling: Practical Aspects of Microphysics in Numerical Simulations. Elsevier, 2024. pp. 323-336

Bibtex

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title = "Integrating astrochemistry in hydrodynamics",

abstract = "Dynamics and astrochemistry in the cosmos frequently, and sometimes strongly, feedback on one another. Therefore, the most predictive simulations of the cosmos should include coupled dynamics + chemistry. The technical details of this coupling are worth considering, in part, because maintaining the conservation of charge and atomic species in a dynamical model requires care, but also because simulating chemistry at every location in a large, multidimensional dynamical model is generally prohibitively expensive. Here, we review how to ensure conservation of species and charge in the most common hydrodynamical numerical methods, how chemistry commonly feeds back onto the dynamics, and present guidelines for how to minimize the cost of modeling coupled chemistry + dynamics.",

keywords = "heating and cooling, Hydrodynamics, numerical methods, radiative transfer",

author = "Troels Haugb{\o}lle and Alessandro Lupi and Jon Ramsey",

year = "2024",

doi = "10.1016/B978-0-32-391746-9.00022-5",

language = "English",

isbn = "9780323972574",

pages = "323--336",

booktitle = "Astrochemical Modeling",

publisher = "Elsevier",

}

RIS

TY - CHAP

T1 - Integrating astrochemistry in hydrodynamics

AU - Haugbølle, Troels

AU - Lupi, Alessandro

AU - Ramsey, Jon

PY - 2024

Y1 - 2024

N2 - Dynamics and astrochemistry in the cosmos frequently, and sometimes strongly, feedback on one another. Therefore, the most predictive simulations of the cosmos should include coupled dynamics + chemistry. The technical details of this coupling are worth considering, in part, because maintaining the conservation of charge and atomic species in a dynamical model requires care, but also because simulating chemistry at every location in a large, multidimensional dynamical model is generally prohibitively expensive. Here, we review how to ensure conservation of species and charge in the most common hydrodynamical numerical methods, how chemistry commonly feeds back onto the dynamics, and present guidelines for how to minimize the cost of modeling coupled chemistry + dynamics.

AB - Dynamics and astrochemistry in the cosmos frequently, and sometimes strongly, feedback on one another. Therefore, the most predictive simulations of the cosmos should include coupled dynamics + chemistry. The technical details of this coupling are worth considering, in part, because maintaining the conservation of charge and atomic species in a dynamical model requires care, but also because simulating chemistry at every location in a large, multidimensional dynamical model is generally prohibitively expensive. Here, we review how to ensure conservation of species and charge in the most common hydrodynamical numerical methods, how chemistry commonly feeds back onto the dynamics, and present guidelines for how to minimize the cost of modeling coupled chemistry + dynamics.

KW - heating and cooling

KW - Hydrodynamics

KW - numerical methods

KW - radiative transfer

U2 - 10.1016/B978-0-32-391746-9.00022-5

DO - 10.1016/B978-0-32-391746-9.00022-5

M3 - Book chapter

AN - SCOPUS:85190007019

SN - 9780323972574

SP - 323

EP - 336

BT - Astrochemical Modeling

PB - Elsevier

ER -

ID: 391158101