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Title: Ultralight Boson Dark Matter and Event Horizon Telescope Observations of M 87 *

Abstract

The initial information from the Event Horizon Telescope (EHT) on M 87 * , the supermassive black hole at the center of the M87 Galaxy, provide direct observational information on its mass, spin, and accretion disk properties. A combination of the EHT data and other constraints provides evidence that M 87 * has a mass ~6.5 × 109 M. EHT also inferred the dimensionless spin parameter |a*| ≳ 0.5 from jet properties; a separate recent analysis using only the light from near M 87 * as measured by the EHT Collaboration found |a*|= 0.9 ± 0.1 . These determinations disfavor ultralight bosons of mass μb ϵ (0.85, 4.6) × 10–21 eV for spin-one bosons and μb ϵ (2.9, 4.6) × 10–21 eV for spin-zero bosons, within the range considered for fuzzy dark matter, invoked to explain dark matter distribution on approximately kiloparsec scales. Future observations of M 87 * could be expected to determine our conclusions.

Authors:
 [1];  [1]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States)
Publication Date:
Research Org.:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1550793
Alternate Identifier(s):
OSTI ID: 1546446
Report Number(s):
BNL-211936-2019-JAAM
Journal ID: ISSN 0031-9007; PRLTAO
Grant/Contract Number:  
SC0012704
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 123; Journal Issue: 2; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; boson; ultralight; dark matter; M87; telescope

Citation Formats

Davoudiasl, Hooman, and Denton, Peter B. Ultralight Boson Dark Matter and Event Horizon Telescope Observations of M87*. United States: N. p., 2019. Web. doi:10.1103/PhysRevLett.123.021102.
Davoudiasl, Hooman, & Denton, Peter B. Ultralight Boson Dark Matter and Event Horizon Telescope Observations of M87*. United States. https://doi.org/10.1103/PhysRevLett.123.021102
Davoudiasl, Hooman, and Denton, Peter B. Wed . "Ultralight Boson Dark Matter and Event Horizon Telescope Observations of M87*". United States. https://doi.org/10.1103/PhysRevLett.123.021102. https://www.osti.gov/servlets/purl/1550793.
@article{osti_1550793,
title = {Ultralight Boson Dark Matter and Event Horizon Telescope Observations of M87*},
author = {Davoudiasl, Hooman and Denton, Peter B.},
abstractNote = {The initial information from the Event Horizon Telescope (EHT) on M87*, the supermassive black hole at the center of the M87 Galaxy, provide direct observational information on its mass, spin, and accretion disk properties. A combination of the EHT data and other constraints provides evidence that M87* has a mass ~6.5 × 109 M⊙. EHT also inferred the dimensionless spin parameter |a*| ≳ 0.5 from jet properties; a separate recent analysis using only the light from near M87* as measured by the EHT Collaboration found |a*|= 0.9 ± 0.1 . These determinations disfavor ultralight bosons of mass μb ϵ (0.85, 4.6) × 10–21 eV for spin-one bosons and μb ϵ (2.9, 4.6) × 10–21 eV for spin-zero bosons, within the range considered for fuzzy dark matter, invoked to explain dark matter distribution on approximately kiloparsec scales. Future observations of M87* could be expected to determine our conclusions.},
doi = {10.1103/PhysRevLett.123.021102},
journal = {Physical Review Letters},
number = 2,
volume = 123,
place = {United States},
year = {Wed Jul 10 00:00:00 EDT 2019},
month = {Wed Jul 10 00:00:00 EDT 2019}
}

Journal Article:

Citation Metrics:
Cited by: 135 works
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Figures / Tables:

FIG. 1 FIG. 1: Regions of parameter space constrained by observations of SMBHs. The orange (blue) region is ruled out for vector (scalar) bosons by M87. Note that the constraints apply to both parity even and parity odd particles. Each constraint is derived using the 1 σ conservative values for the massmore » and spin, and the shaded band on the left of each region represents the size of the theoretical uncertainty. The green region is the constraint on vector bosons from Ark 120 [18] which cannot constrain scalars. The region preferred by fuzzy DM is shown in gray.« less

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    Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.