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ZENODO
Conference object . 2016
License: CC BY
Data sources: Datacite
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ZENODO
Other literature type . 2016
License: CC BY
Data sources: ZENODO
https://dx.doi.org/10.5281/zen...
Other literature type
Data sources: Microsoft Academic Graph
https://dx.doi.org/10.5281/zen...
Other literature type
Data sources: Microsoft Academic Graph
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The Phantom Sph Code

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 15 Jul 2016Publisher:Zenodo
Authors: Price, Daniel; Wurster, James; Nixon, Chris;

doi: 10.5281/zenodo.58009

The Phantom Sph Code

Abstract

I will present the capabilities of the Phantom SPH code for global simulations of dust and gas in protoplanetary discs. I will present our new algorithms for simulating both small and large grains in discs, as well as our progress towards simulating evolving grain populations and coupling with radiation. Finally, I will discuss our recent applications to HL Tau and the physics of dust gap opening.

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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