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A. Gamboa

10 papers hereh-index 8179 citations28 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author6

Across the 10 of 10 papers where every author was matched, so the position is known.

fields
  • gr-qc9
  • astro-ph.HE1
same name
  • A. Gamboa — 20 papers
  • A. Gamboa — 6 papers, h 3
  • A. Gamboa — 5 papers
  • A. Gamboa — 3 papers
  • A. Gamboa — 2 papers, h 15
  • A. Gamboa — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20242026
most citedAccurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM

57 citations · 116 across the 10 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

gr-qc2024★ 28 cited

Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM

Aldo Gamboa, Mohammed Khalil, Alessandra Buonanno

Accurate waveform models for coalescing binaries on eccentric orbits are crucial for avoiding biases in the analysis of eccentric gravitational-wave signals. The effective-one-body…

gr-qc2024★ 57 cited

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM

Aldo Gamboa, Alessandra Buonanno, Raffi Enficiaud +9

The measurement of orbital eccentricity in gravitational-wave (GW) signals will provide unique insights into the astrophysical origin of binary systems, while ignoring eccentricity…

gr-qc2024★ 13 cited

Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models

Guglielmo Faggioli, Maarten van de Meent, Alessandra Buonanno +3

In this work, we test an effective-one-body radiation-reaction force for eccentric planar orbits of a test mass in a Kerr background, which contains third-order post-Newtonian (PN)…

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