2023MNRAS.519.6008B


Query : 2023MNRAS.519.6008B

2023MNRAS.519.6008B - Mon. Not. R. Astron. Soc., 519, 6008-6019 (2023/March-2)

Tracking the origin of black holes with the stochastic gravitational wave background popcorn signal.

BRAGLIA M., GARCIA-BELLIDO J. and KUROYANAGI S.

Abstract (from CDS):

Unresolved sources of gravitational waves (GWs) produced by the merger of a binary of black holes at cosmological distances combine into a stochastic background. Such a background is in the continuous or popcorn regime, depending on whether the GW rate is high enough so that two or more events overlap in the same frequency band. These two regimes respectively correspond to large and small values of the so-called duty cycle. We study the detection regime of the background in models of primordial black holes (PBHs) and compare it to the one produced by black holes of stellar origin. Focusing on ground-based detectors, we show that the duty cycle of the PBH-origin background is larger than that of astrophysical black holes because of differences in their mass function and the merger rate. Our study opens up the possibility to learn about the primordial or astrophysical nature of black hole populations by examining the statistical properties of the stochastic background.

Abstract Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - gravitational waves

Simbad objects: 1

goto Full paper

goto View the references in ADS

Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Eridanus II G 03 44 21.1 -43 32 00           ~ 216 0

Query : 2023MNRAS.519.6008B

Basic data :
NAME Eridanus II -- Galaxy
Other object types:
otypes_help
G (2015ApJ,[BDB2015])
ICRS coord. (ep=J2000) :
03 44 21.1 -43 32 00 (Optical) [ ] D 2015ApJ...805..130K
FK4 coord. (ep=B1950 eq=1950) :
03 42 40.0 -43 41 22 [ ]
Gal coord. (ep=J2000) :
249.7817 -51.6464 [ ]
Proper motions mas/yr :
0.16 0.15 [0.24 0.26 90] C 2019ApJ...875...77P
Morphological type:
-3 D 2018MNRAS.479.4136K
SIMBAD within arcmin
Overlay Simbad points in this preview
Back
All CDSPortal (CDSPortal)

Send to sendBySAMP sendBySAMP

sedIcon
within arcsec sed-help-icon

Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 136
Display criteria :

Identifiers (3) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

NAME Eri II NAME Eridanus II [BDB2015] DES J0344.3-4331

References (216 between 1850 and 2026) (Total 216)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
Follow new references on this object
                Reference summaries :

                from: to:

                 or select by : (not exhaustive, explanation here)


Collections of Measurements Description of Measurements

Distance : 2    PM : 1   

   


External archives :

Search by coordinates in Vizier (radius: 5 arcsec)


Annotations :
Annotations allow a user to add a note or report an error concerning the astronomical object and its data. It requires registration to post a note. See description .
Please, have a look at Best practices. The list of all annotations to SIMBAD objects can be found here .

The annotation server is currently not available. Sorry for any inconvenience


To bookmark this query, right click on this link: simbad:objects in 2023MNRAS.519.6008B and select 'bookmark this link' or equivalent in the popup menu