FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2907223768> ?p ?o ?g. }

• W2907223768 endingPage "2308" @default.
• W2907223768 startingPage "2296" @default.
• W2907223768 abstract "We explore in situ formation and subsequent evolution of close-in super-Earths and mini-Neptunes. We adopt a steady-state inner protoplanetary gas disc structure that arises from viscous accretion due to the magneto-rotational instability (MRI). We consider the evolution of dust in the inner disc, including growth, radial drift and fragmentation, and find that dust particles that radially drift into the inner disc fragment severely due to the MRI-induced turbulence. This result has two consequences: (1) radial drift of grains within the inner disc is quenched, leading to an enhancement of dust in the inner regions which scales as dust-to-gas-mass-flux-ratio at ~1 AU; (2) however, despite this enhancement, planetesimal formation is impeded by the small grain size. Nevertheless, assuming that planetary cores are present in the inner disc, we then investigate the accretion of atmospheres onto cores and their subsequent photoevaporation. We then compare our results to the observed exoplanet mass-radius relationship. We find that: (1) the low gas surface densities and high temperatures in the inner disc reduce gas accretion onto cores compared to the minimum mass solar nebula, preventing the cores from growing into hot Jupiters, in agreement with the data; (2) however, our predicted envelope masses are still typically larger than observed ones. Finally, we sketch a qualitative picture of how grains may grow and planetesimals form in the inner disc if grain effects on the ionization levels and the MRI and the back-reaction of the dust on the gas (both neglected in our calculations) are accounted for." @default.
• W2907223768 created "2019-01-11" @default.
• W2907223768 creator A5017575956 @default.
• W2907223768 creator A5032539052 @default.
• W2907223768 creator A5044437031 @default.
• W2907223768 date "2019-01-05" @default.
• W2907223768 modified "2023-09-25" @default.
• W2907223768 title "Close-in Super-Earths: The first and the last stages of planet formation in an MRI-accreting disc" @default.
• W2907223768 cites W1781644248 @default.
• W2907223768 cites W1829925112 @default.
• W2907223768 cites W1844505821 @default.
• W2907223768 cites W1966383761 @default.
• W2907223768 cites W1970201714 @default.
• W2907223768 cites W1970964877 @default.
• W2907223768 cites W1973899631 @default.
• W2907223768 cites W1987005932 @default.
• W2907223768 cites W1990714769 @default.
• W2907223768 cites W2000421598 @default.
• W2907223768 cites W2000657683 @default.
• W2907223768 cites W2003334213 @default.
• W2907223768 cites W2004819229 @default.
• W2907223768 cites W2005561978 @default.
• W2907223768 cites W2006491802 @default.
• W2907223768 cites W2011177045 @default.
• W2907223768 cites W2021293208 @default.
• W2907223768 cites W2023381428 @default.
• W2907223768 cites W2029003601 @default.
• W2907223768 cites W2041172302 @default.
• W2907223768 cites W2043827471 @default.
• W2907223768 cites W2045556557 @default.
• W2907223768 cites W2047176025 @default.
• W2907223768 cites W2049013365 @default.
• W2907223768 cites W2049527803 @default.
• W2907223768 cites W2052352548 @default.
• W2907223768 cites W2056624052 @default.
• W2907223768 cites W2059897684 @default.
• W2907223768 cites W2062197591 @default.
• W2907223768 cites W2066986330 @default.
• W2907223768 cites W2068008066 @default.
• W2907223768 cites W2068433364 @default.
• W2907223768 cites W2079333065 @default.
• W2907223768 cites W2083936836 @default.
• W2907223768 cites W2088449621 @default.
• W2907223768 cites W2096258061 @default.
• W2907223768 cites W2107163299 @default.
• W2907223768 cites W2107656875 @default.
• W2907223768 cites W2130754528 @default.
• W2907223768 cites W2132117032 @default.
• W2907223768 cites W2132519231 @default.
• W2907223768 cites W2141938416 @default.
• W2907223768 cites W2149470802 @default.
• W2907223768 cites W2149520698 @default.
• W2907223768 cites W2289070232 @default.
• W2907223768 cites W2326850392 @default.
• W2907223768 cites W2515740491 @default.
• W2907223768 cites W2525760866 @default.
• W2907223768 cites W2549068182 @default.
• W2907223768 cites W2606686133 @default.
• W2907223768 cites W2615268591 @default.
• W2907223768 cites W2737465989 @default.
• W2907223768 cites W2743656798 @default.
• W2907223768 cites W2762105321 @default.
• W2907223768 cites W2763533228 @default.
• W2907223768 cites W2781319575 @default.
• W2907223768 cites W2791940915 @default.
• W2907223768 cites W2804190688 @default.
• W2907223768 cites W2947592794 @default.
• W2907223768 cites W2963604282 @default.
• W2907223768 cites W3098015989 @default.
• W2907223768 cites W3098251033 @default.
• W2907223768 cites W3098896129 @default.
• W2907223768 cites W3099058670 @default.
• W2907223768 cites W3099093368 @default.
• W2907223768 cites W3099213932 @default.
• W2907223768 cites W3099362172 @default.
• W2907223768 cites W3099492014 @default.
• W2907223768 cites W3099599729 @default.
• W2907223768 cites W3099749551 @default.
• W2907223768 cites W3099966931 @default.
• W2907223768 cites W3100406661 @default.
• W2907223768 cites W3100530613 @default.
• W2907223768 cites W3100845463 @default.
• W2907223768 cites W3100933337 @default.
• W2907223768 cites W3100998258 @default.
• W2907223768 cites W3101377879 @default.
• W2907223768 cites W3101861203 @default.
• W2907223768 cites W3101909195 @default.
• W2907223768 cites W3101918238 @default.
• W2907223768 cites W3102094901 @default.
• W2907223768 cites W3102817586 @default.
• W2907223768 cites W3103485317 @default.
• W2907223768 cites W3103791428 @default.
• W2907223768 cites W3103893120 @default.
• W2907223768 cites W3103922012 @default.
• W2907223768 cites W3104207897 @default.
• W2907223768 cites W3104879793 @default.
• W2907223768 cites W3104957872 @default.
• W2907223768 cites W3105362078 @default.

• next