Gennaro D'Angelo

Dr. Gennaro D'Angelo

orcid

Research Focus & Metrics

Academic Career Length

26Years (2001-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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22 June 2006 in Monthly Notices of the Royal Astronomical Society
Verified
Journal Article
Open access
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MVM. De Val-Borro
M. De Val-Borro
RER. G. Edgar
R. G. Edgar
PAP. Artymowicz
P. Artymowicz
PCP. Ciecielag
P. Ciecielag
PCP. Cresswell
P. Cresswell
RSR. Speith
R. Speith
We perform numerical simulations of a disc–planet system using various grid-based and smoothed particle hydrodynamics (SPH) codes. The tests are run

1 February 2009 in Icarus
Verified
Journal Article
Closed access
JLJack J. Lissauer
Jack J. Lissauer
OHOlenka Hubickyj
Olenka Hubickyj
GDGennaro D'Angelo
Gennaro D'Angelo
PBPeter Bodenheimer
Peter Bodenheimer

20 March 2003 in The Astrophysical Journal
Verified
Journal Article
Closed access
GDGennaro D'Angelo
Gennaro D'Angelo
WKWilly Kley
Willy Kley
THThomas Henning
Thomas Henning
We investigate the evolution of protoplanets with different masses embedded in an accretion disk, via global fully three-dimensional hydrodynamical simulations. We consider a range of planetary masses extending from one and a half Earth's masses up to one Jupiter's mass, and we take into account physically realistic gravitational potentials of forming planets. In order to calculate accurately the gravitational torques exerted by disk material and to investigate the accretion process onto the planet, the flow dynamics has to be thoroughly resolved on long as well as short length scales. We achieve this strict resolution requirement by applying a nested-grid refinement technique which allows to greatly enhance the local resolution. Our results from altogether 51 simulations show that for large planetary masses, approximately above a tenth of the Jupiter's mass, migration rates are relatively constant, as expected in type II migration regime and in good agreement with previous two-dimensional calculations. In a range between seven and fifteen Earth's masses, we find a dependency of the migration speed on the planetary mass that yields time scales considerably longer than those predicted by linear analytical theories. This property may be important in determining the overall orbital evolution of protoplanets. The growth time scale is minimum around twenty Earth-masses, but it rapidly increases for both smaller and larger mass values. Significant differences between two- and three-dimensional calculations are found in particular for objects with masses smaller than ten Earth-masses. We also derive an analytical approximation for the numerically computed mass growth rates

15 April 2002 in Astronomy & Astrophysics
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Journal Article
Open access
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GDGennaro D'Angelo
Gennaro D'Angelo
THT. Henning
T. Henning
WKW. Kley
W. Kley
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

26 June 2007 in Astronomy & Astrophysics
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Journal Article
Open access
PDF file
MVM. de Val-Borro
M. de Val-Borro
PAP. Artymowicz
P. Artymowicz
GDGennaro D'Angelo
Gennaro D'Angelo
APA. Peplinski
A. Peplinski
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysics

4 November 2010 in The Astrophysical Journal
Verified
Journal Article
Closed access
GDGennaro D'Angelo
Gennaro D'Angelo
SLStephen H. Lubow
Stephen H. Lubow