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dc.date.accessioned2020-10-05T18:16:55Z
dc.date.available2020-10-05T18:16:55Z
dc.date.created2020-09-30T15:36:22Z
dc.date.issued2020
dc.identifier.citationMina, Mattia Mota, David Winther, Hans Arnold . SCALAR: an AMR code to simulate axion-like dark matter models. Astronomy and Astrophysics. 2020, 641
dc.identifier.urihttp://hdl.handle.net/10852/80223
dc.description.abstractWe present a new code,SCALAR, based on the high-resolution hydrodynamics andN-body codeRAMSES, to solve the Schrödingerequation on adaptive refined meshes. The code is intended to be used to simulate axion or fuzzy dark matter models where theevolution of the dark matter component is determined by a coupled Schrödinger-Poisson equation, but it can also be used as a stand-alone solver for both linear and non-linear Schrödinger equations with any given external potential. This paper describes the numericalimplementation of our solver and presents tests to demonstrate how accurately it operates.
dc.languageEN
dc.relation.ispartofMina, Mattia (2020) Cosmology at small scales: ultra-light dark matter and baryon cycles in galaxies. Doctoral thesis http://hdl.handle.net/10852/80876
dc.relation.urihttp://hdl.handle.net/10852/80876
dc.titleSCALAR: an AMR code to simulate axion-like dark matter models
dc.typeJournal article
dc.creator.authorMina, Mattia
dc.creator.authorMota, David
dc.creator.authorWinther, Hans Arnold
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1835746
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy and Astrophysics&rft.volume=641&rft.spage=&rft.date=2020
dc.identifier.jtitleAstronomy and Astrophysics
dc.identifier.volume641
dc.identifier.pagecount16
dc.identifier.doi0004-6361/201936272
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201936272
dc.identifier.urnURN:NBN:no-83326
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-6361
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/80223/1/aa36272-19.pdf
dc.type.versionPublishedVersion
cristin.articleidA107
dc.relation.projectNFR/287772


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