D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 73 Citations 20,256 269 World Ranking 2951 National Ranking 151

Overview

What is she best known for?

The fields of study she is best known for:

  • Astronomy
  • Astrophysics
  • Galaxy

Her primary areas of study are Astrophysics, Gravitational wave, Supernova, Metallicity and Stars. Michela Mapelli combines topics linked to Astronomy with her work on Astrophysics. Her study focuses on the intersection of Supernova and fields such as Common envelope with connections in the field of Eddington luminosity.

While the research belongs to areas of Metallicity, Michela Mapelli spends her time largely on the problem of Stellar evolution, intersecting her research to questions surrounding Stellar black hole. Her Stars research focuses on subjects like Galaxy, which are linked to Ejecta, Spectral line, Nucleosynthesis and Gamma-ray burst. Her Compact star study, which is part of a larger body of work in Neutron star, is frequently linked to Root mean square, bridging the gap between disciplines.

Her most cited work include:

  • Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger (478 citations)
  • GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙ (463 citations)
  • Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo (439 citations)

What are the main themes of her work throughout her whole career to date?

Michela Mapelli mostly deals with Astrophysics, Stars, Astronomy, Galaxy and Gravitational wave. Metallicity, Black hole, Neutron star, Supernova and LIGO are the subjects of her Astrophysics studies. Her biological study spans a wide range of topics, including X-ray, Stellar wind, Stellar evolution, Mass gap and Young star.

Michela Mapelli interconnects Gamma-ray burst and Pulsar in the investigation of issues within Neutron star. Her work on Star cluster and Galactic Center as part of general Stars research is often related to Mass spectrum and Angular momentum, thus linking different fields of science. Her work investigates the relationship between Gravitational wave and topics such as Redshift that intersect with problems in Dark matter.

She most often published in these fields:

  • Astrophysics (116.34%)
  • Stars (46.76%)
  • Astronomy (41.13%)

What were the highlights of her more recent work (between 2019-2021)?

  • Astrophysics (116.34%)
  • Gravitational wave (43.38%)
  • LIGO (25.63%)

In recent papers she was focusing on the following fields of study:

Her scientific interests lie mostly in Astrophysics, Gravitational wave, LIGO, Binary black hole and Neutron star. Star cluster, Metallicity, Stars, Galaxy and Black hole are the primary areas of interest in her Astrophysics study. Her study brings together the fields of Supernova and Stars.

Radius is closely connected to Mass ratio in her research, which is encompassed under the umbrella topic of Gravitational wave. Her studies deal with areas such as Gamma-ray burst and Dimensionless quantity as well as LIGO. Her Binary black hole study combines topics in areas such as Redshift, Common envelope and Binary star.

Between 2019 and 2021, her most popular works were:

  • GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙ (463 citations)
  • GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$ (389 citations)
  • GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object (356 citations)

In her most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Galaxy

Her primary scientific interests are in Astrophysics, Gravitational wave, Neutron star, LIGO and Stars. Her General relativity research extends to Astrophysics, which is thematically connected. Her work on Mass ratio expands to the thematically related Gravitational wave.

Her Neutron star study integrates concerns from other disciplines, such as Coalescence, Mass distribution and First observation of gravitational waves. Her work in the fields of Star cluster and Metallicity overlaps with other areas such as Mass spectrum and Equation of state. As a part of the same scientific family, Michela Mapelli mostly works in the field of Binary black hole, focusing on Redshift and, on occasion, Intermediate-mass black hole.

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$

B. P. Abbott;R. Abbott.
arXiv: High Energy Astrophysical Phenomena (2020)

1102 Citations

GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M O

B. P. Abbott;R. Abbott;T. D. Abbott;S. Abraham.
The Astrophysical Journal (2020)

856 Citations

Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo

B. P. Abbott;R. Abbott.
arXiv: High Energy Astrophysical Phenomena (2018)

663 Citations

Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger

E. Pian;P. D'Avanzo;S. Benetti;M. Branchesi.
Nature (2017)

549 Citations

GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

R. Abbott;T. D. Abbott.
arXiv: High Energy Astrophysical Phenomena (2020)

475 Citations

GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object

R. Abbott;T. D. Abbott;S. Abraham;F. Acernese.
The Astrophysical Journal (2020)

376 Citations

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

R. Abbott;R. Abbott;T.D. Abbott;S. Abraham;F. Acernese.
Physical Review X (2021)

348 Citations

GW190521: A Binary Black Hole Merger with a Total Mass of 150 M

R. Abbott;T. D. Abbott;S. Abraham;F. Acernese.
Physical Review Letters (2020)

340 Citations

The mass spectrum of compact remnants from the parsec stellar evolution tracks

Mario Spera;Michela Mapelli;Michela Mapelli;Alessandro Bressan;Alessandro Bressan.
Monthly Notices of the Royal Astronomical Society (2015)

260 Citations

Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog

R. Abbott;T. D. Abbott.
arXiv: High Energy Astrophysical Phenomena (2020)

252 Citations

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