FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3204282983> ?p ?o ?g. }

• W3204282983 endingPage "156" @default.
• W3204282983 startingPage "156" @default.
• W3204282983 abstract "The abundance and distribution of solids inside the Hill sphere are central to our understanding of the giant planet dichotomy. Here, we present a three-dimensional characterization of the dust density, mass flux, and mean opacities in the envelope of sub-thermal and super-thermal mass planets. We simulate the dynamics of multiple dust species in a global protoplanetary disk model accounting for dust feedback. We find that the meridional flows do not effectively stir dust grains at scales of the Bondi sphere. Thus the dust-settling driven by the stellar gravitational potential sets the latitudinal dust density gradient within the planet envelope. Not only does the planet's potential enhance this gradient, but also the spiral wakes serve as another source of asymmetry. These asymmetries substantially alter the inferred mean Rosseland and Planck opacities. In cases with the moderate-to-strong dust settling, the opacity gradient can range from a few percent to more than two orders of magnitude between the mid-plane and the polar regions of the Bondi sphere. Finally, we show that this strong latitudinal opacity gradient can introduce a transition between optically thick and thin regimes at the scales of the planet envelope. We suggest that this transition is likely to occur when the equilibrium scale height of hundred-micron-sized particles is smaller than the Hill radius of the forming planet. This work calls into question the adoption of a constant opacity derived from well-mixed distributions and demonstrates the need for global radiation hydrodynamics models of giant planet formation which account for dust dynamics." @default.
• W3204282983 created "2021-10-11" @default.
• W3204282983 creator A5047859538 @default.
• W3204282983 creator A5062895011 @default.
• W3204282983 creator A5066165480 @default.
• W3204282983 date "2022-04-01" @default.
• W3204282983 modified "2023-09-26" @default.
• W3204282983 title "The 3D Dust and Opacity Distribution of Protoplanets in Multifluid Global Simulations" @default.
• W3204282983 cites W1623184197 @default.
• W3204282983 cites W1829925112 @default.
• W3204282983 cites W1964429329 @default.
• W3204282983 cites W1968443772 @default.
• W3204282983 cites W1978204777 @default.
• W3204282983 cites W1987345881 @default.
• W3204282983 cites W1990479198 @default.
• W3204282983 cites W2006491802 @default.
• W3204282983 cites W2023097392 @default.
• W3204282983 cites W2037345895 @default.
• W3204282983 cites W2041389756 @default.
• W3204282983 cites W2050870661 @default.
• W3204282983 cites W2064179933 @default.
• W3204282983 cites W2069325316 @default.
• W3204282983 cites W2083936836 @default.
• W3204282983 cites W2085447852 @default.
• W3204282983 cites W2099066749 @default.
• W3204282983 cites W2106503697 @default.
• W3204282983 cites W2113436460 @default.
• W3204282983 cites W2115618550 @default.
• W3204282983 cites W2140611633 @default.
• W3204282983 cites W2141244722 @default.
• W3204282983 cites W2141938416 @default.
• W3204282983 cites W2149520698 @default.
• W3204282983 cites W2155063694 @default.
• W3204282983 cites W2162462253 @default.
• W3204282983 cites W2168570318 @default.
• W3204282983 cites W2400070749 @default.
• W3204282983 cites W2604436716 @default.
• W3204282983 cites W2606081896 @default.
• W3204282983 cites W2737465989 @default.
• W3204282983 cites W2784741468 @default.
• W3204282983 cites W2793560755 @default.
• W3204282983 cites W2798613580 @default.
• W3204282983 cites W2807085682 @default.
• W3204282983 cites W2810591005 @default.
• W3204282983 cites W2897198037 @default.
• W3204282983 cites W2904495956 @default.
• W3204282983 cites W2943886700 @default.
• W3204282983 cites W2951022004 @default.
• W3204282983 cites W2960204344 @default.
• W3204282983 cites W2974039287 @default.
• W3204282983 cites W3007463484 @default.
• W3204282983 cites W3098022595 @default.
• W3204282983 cites W3098077360 @default.
• W3204282983 cites W3099791366 @default.
• W3204282983 cites W3099926431 @default.
• W3204282983 cites W3100059172 @default.
• W3204282983 cites W3100401297 @default.
• W3204282983 cites W3100507371 @default.
• W3204282983 cites W3100764049 @default.
• W3204282983 cites W3101563883 @default.
• W3204282983 cites W3101698842 @default.
• W3204282983 cites W3102230464 @default.
• W3204282983 cites W3103230860 @default.
• W3204282983 cites W3103603022 @default.
• W3204282983 cites W3105414201 @default.
• W3204282983 cites W3105659461 @default.
• W3204282983 cites W3105707728 @default.
• W3204282983 cites W3105727434 @default.
• W3204282983 cites W3105727738 @default.
• W3204282983 cites W3106540147 @default.
• W3204282983 cites W3124935840 @default.
• W3204282983 cites W3127279059 @default.
• W3204282983 cites W3136618726 @default.
• W3204282983 cites W3157495290 @default.
• W3204282983 cites W3163711189 @default.
• W3204282983 cites W3174186536 @default.
• W3204282983 cites W3185923429 @default.
• W3204282983 cites W3204941133 @default.
• W3204282983 cites W4292332867 @default.
• W3204282983 doi "https://doi.org/10.3847/1538-4357/ac5899" @default.
• W3204282983 hasPublicationYear "2022" @default.
• W3204282983 type Work @default.
• W3204282983 sameAs 3204282983 @default.
• W3204282983 citedByCount "6" @default.
• W3204282983 countsByYear W32042829832022 @default.
• W3204282983 countsByYear W32042829832023 @default.
• W3204282983 crossrefType "journal-article" @default.
• W3204282983 hasAuthorship W3204282983A5047859538 @default.
• W3204282983 hasAuthorship W3204282983A5062895011 @default.
• W3204282983 hasAuthorship W3204282983A5066165480 @default.
• W3204282983 hasBestOaLocation W32042829831 @default.
• W3204282983 hasConcept C120665830 @default.
• W3204282983 hasConcept C121332964 @default.
• W3204282983 hasConcept C1276947 @default.
• W3204282983 hasConcept C12853656 @default.
• W3204282983 hasConcept C173209714 @default.
• W3204282983 hasConcept C178635117 @default.
• W3204282983 hasConcept C2780909310 @default.

• next