Binary Evolution in Galactic Nuclei

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Stellar Astronomy".

Deadline for manuscript submissions: closed (1 May 2022) | Viewed by 1817

Special Issue Editors

Max Planck Institute for Astrophysics, Garching bei Munchen, Germany
Interests: Computational astrophysics; gravitational dynamics; stellar and binary evolution; long-term evolution of multi-star (binary, triple, and quadruple) systems during all stages of stellar evolution, in low and high-density environments (from the field to galactic nuclei); applications in gravitational wave sources, supernovae, and (exo)planets

E-Mail Website
Guest Editor
Department of Physics, Università di Roma "La Sapienza", 00185 Rome, Italy
Interests: theoretical astrophysics; gravitational physics; computational astrophysics; numerical methods

Special Issue Information

Dear Colleagues,

Galactic nuclei and the supermassive black holes (SMBHs) that they often contain have received much attention in the last decade, especially with the recent detection of gravitational waves (GWs) from mergers of stellar-mass BHs that could reside in these systems. One particularly interesting consideration is that an SMBH can secularly perturb and accelerate the merger of stellar-mass BH binaries orbiting around it through the (eccentric) von Zeipel-Lidov-Kozai mechanism. Although the latter mechanism has been studied in the literature before, many complications have been often ignored, including interactions of the binary with other stars in the galactic nucleus (e.g., through processes known as resonant relaxation, and through triaxiality of the cluster), and pre-compact object stellar and binary evolution.

The goal of this Special Issue is to consolidate recent advances in the field of binary dynamics and evolution. Issue topics include, but are not limited to:

1. gravitational dynamics of binaries near SMBHs

2. perturbations from other stars and compact objects (including fly-bys, correlated encounters, and non-spherically-symmetric potentials)

3. the impact of stellar evolution

4. gravitational wave signals from binaries near SMBHs

5. other implications of binary mergers such as supernovae and blue straggler formation

Dr. Adrian Hamers
Prof. Dr. Roberto Capuzzo Dolcetta
Guest Editors

References

1. Binary Dynamics Near a Massive Black Hole
https://ui.adsabs.harvard.edu/abs/2009ApJ...700.1933H/abstract

2. Greatly Enhanced Merger Rates of Compact-object Binaries in Non-spherical Nuclear Star Clusters
https://ui.adsabs.harvard.edu/abs/2017ApJ...846..146P/abstract

3. Black Hole Mergers in Galactic Nuclei Induced by the Eccentric Kozai-Lidov Effect
https://ui.adsabs.harvard.edu/abs/2018ApJ...856..140H/abstract

4. Eccentric Black Hole Gravitational-wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters
https://ui.adsabs.harvard.edu/abs/2018ApJ...860....5G/abstract

5. Black hole and neutron star mergers in galactic nuclei
https://ui.adsabs.harvard.edu/abs/2019MNRAS.488...47F/abstract

Manuscript Submission Information

Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.

Submitted manuscripts should not have been published previously, nor be under consideration for publication elsewhere (except conference proceedings papers). All manuscripts are thoroughly refereed through a single-blind peer-review process. A guide for authors and other relevant information for submission of manuscripts is available on the Instructions for Authors page. Universe is an international peer-reviewed open access monthly journal published by MDPI.

Please visit the Instructions for Authors page before submitting a manuscript. Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.

Keywords

  • (Supermassive) black holes
  • galactic nuclei
  • gravitational dynamics
  • stellar and binary evolution
  • gravitational waves
  • cluster dynamics

Published Papers (1 paper)

Order results
Result details
Select all
Export citation of selected articles as:

Review

65 pages, 3005 KiB  
Review
Quiescent and Active Galactic Nuclei as Factories of Merging Compact Objects in the Era of Gravitational Wave Astronomy
by Manuel Arca Sedda, Smadar Naoz and Bence Kocsis
Universe 2023, 9(3), 138; https://doi.org/10.3390/universe9030138 - 06 Mar 2023
Cited by 14 | Viewed by 1367
Abstract
Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded by a dense nuclear cluster (NC), represent extreme environments that house a complex interplay of many physical processes that uniquely affect stellar formation, evolution, and dynamics. The discovery of gravitational waves (GWs) [...] Read more.
Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded by a dense nuclear cluster (NC), represent extreme environments that house a complex interplay of many physical processes that uniquely affect stellar formation, evolution, and dynamics. The discovery of gravitational waves (GWs) emitted by merging black holes (BHs) and neutron stars (NSs), funnelled a huge amount of work focused on understanding how compact object binaries (COBs) can pair up and merge together. Here, we review from a theoretical standpoint how different mechanisms concur with the formation, evolution, and merger of COBs around quiescent SMBHs and active galactic nuclei (AGNs), summarising the main predictions for current and future (GW) detections and outlining the possible features that can clearly mark a galactic nuclei origin. Full article
(This article belongs to the Special Issue Binary Evolution in Galactic Nuclei)
Show Figures

Figure 1

Back to TopTop