Matches in SemOpenAlex for { <https://semopenalex.org/work/W4292213306> ?p ?o ?g. }
- W4292213306 endingPage "35" @default.
- W4292213306 startingPage "35" @default.
- W4292213306 abstract "Many processes during the evolution of protoplanetary disks and during planet formation are highly sensitive to the sizes of dust particles that are present in the disk: The efficiency of dust accretion in the disk and volatile transport on dust particles, gravoturbulent instabilities leading to the formation of planetesimals, or the accretion of pebbles onto large planetary embryos to form giant planets are typical examples of processes that depend on the sizes of the dust particles involved. Furthermore, radiative properties like absorption or scattering opacities depend on the particle sizes. To interpret observations of dust in protoplanetary disks, a proper estimate of the dust particle sizes is needed. We present DustPy - A Python package to simulate dust evolution in protoplanetary disks. DustPy solves gas and dust transport including viscous advection and diffusion as well as collisional growth of dust particles. DustPy is written with a modular concept, such that every aspect of the model can be easily modified or extended to allow for a multitude of research opportunities." @default.
- W4292213306 created "2022-08-18" @default.
- W4292213306 creator A5016174491 @default.
- W4292213306 creator A5031287880 @default.
- W4292213306 date "2022-08-01" @default.
- W4292213306 modified "2023-09-30" @default.
- W4292213306 title "DustPy: A Python Package for Dust Evolution in Protoplanetary Disks" @default.
- W4292213306 cites W1978693245 @default.
- W4292213306 cites W2000657683 @default.
- W4292213306 cites W2001871416 @default.
- W4292213306 cites W2006491802 @default.
- W4292213306 cites W2023381428 @default.
- W4292213306 cites W2034133160 @default.
- W4292213306 cites W2037032330 @default.
- W4292213306 cites W2041172302 @default.
- W4292213306 cites W2043595416 @default.
- W4292213306 cites W2044830669 @default.
- W4292213306 cites W2052883156 @default.
- W4292213306 cites W2057006726 @default.
- W4292213306 cites W2065971335 @default.
- W4292213306 cites W2066319384 @default.
- W4292213306 cites W2069325316 @default.
- W4292213306 cites W2080480291 @default.
- W4292213306 cites W2086889382 @default.
- W4292213306 cites W2100328029 @default.
- W4292213306 cites W2116952160 @default.
- W4292213306 cites W2131427944 @default.
- W4292213306 cites W2575362938 @default.
- W4292213306 cites W2735280519 @default.
- W4292213306 cites W2917825507 @default.
- W4292213306 cites W3016058354 @default.
- W4292213306 cites W3090249879 @default.
- W4292213306 cites W3098002080 @default.
- W4292213306 cites W3099300400 @default.
- W4292213306 cites W3099754515 @default.
- W4292213306 cites W3099860744 @default.
- W4292213306 cites W3100933549 @default.
- W4292213306 cites W3100990910 @default.
- W4292213306 cites W3100998258 @default.
- W4292213306 cites W3102746459 @default.
- W4292213306 cites W3103145119 @default.
- W4292213306 cites W3104010814 @default.
- W4292213306 cites W3104970453 @default.
- W4292213306 cites W3105572205 @default.
- W4292213306 cites W3105743825 @default.
- W4292213306 cites W3105870319 @default.
- W4292213306 cites W3106853966 @default.
- W4292213306 cites W3109307471 @default.
- W4292213306 cites W3122214647 @default.
- W4292213306 cites W3123804069 @default.
- W4292213306 cites W3147751559 @default.
- W4292213306 cites W3207547691 @default.
- W4292213306 cites W3209233181 @default.
- W4292213306 cites W4205787579 @default.
- W4292213306 cites W4250669841 @default.
- W4292213306 cites W4289773239 @default.
- W4292213306 cites W4289776269 @default.
- W4292213306 cites W4300192594 @default.
- W4292213306 cites W4376595747 @default.
- W4292213306 doi "https://doi.org/10.3847/1538-4357/ac7d58" @default.
- W4292213306 hasPublicationYear "2022" @default.
- W4292213306 type Work @default.
- W4292213306 citedByCount "11" @default.
- W4292213306 countsByYear W42922133062022 @default.
- W4292213306 countsByYear W42922133062023 @default.
- W4292213306 crossrefType "journal-article" @default.
- W4292213306 hasAuthorship W4292213306A5016174491 @default.
- W4292213306 hasAuthorship W4292213306A5031287880 @default.
- W4292213306 hasBestOaLocation W42922133061 @default.
- W4292213306 hasConcept C100905312 @default.
- W4292213306 hasConcept C121332964 @default.
- W4292213306 hasConcept C163479331 @default.
- W4292213306 hasConcept C190841160 @default.
- W4292213306 hasConcept C2776401274 @default.
- W4292213306 hasConcept C2780909310 @default.
- W4292213306 hasConcept C32449521 @default.
- W4292213306 hasConcept C44870925 @default.
- W4292213306 hasConcept C5072599 @default.
- W4292213306 hasConcept C51244244 @default.
- W4292213306 hasConcept C539450922 @default.
- W4292213306 hasConcept C62520636 @default.
- W4292213306 hasConcept C66279824 @default.
- W4292213306 hasConcept C73411000 @default.
- W4292213306 hasConcept C74902906 @default.
- W4292213306 hasConcept C75876914 @default.
- W4292213306 hasConcept C87355193 @default.
- W4292213306 hasConcept C8865038 @default.
- W4292213306 hasConcept C97355855 @default.
- W4292213306 hasConceptScore W4292213306C100905312 @default.
- W4292213306 hasConceptScore W4292213306C121332964 @default.
- W4292213306 hasConceptScore W4292213306C163479331 @default.
- W4292213306 hasConceptScore W4292213306C190841160 @default.
- W4292213306 hasConceptScore W4292213306C2776401274 @default.
- W4292213306 hasConceptScore W4292213306C2780909310 @default.
- W4292213306 hasConceptScore W4292213306C32449521 @default.
- W4292213306 hasConceptScore W4292213306C44870925 @default.
- W4292213306 hasConceptScore W4292213306C5072599 @default.
- W4292213306 hasConceptScore W4292213306C51244244 @default.