QSO strong gravitational lensing and the detection of dark halos

Research output: Contribution to journalArticle

Abstract

We present recent results concerning the possibility to detect dark satellites around galaxies using QSO strong gravitational lensing. Combining high resolution hydrodynamical simulations of galaxy formation and analytic studies we show that current QSO observations data do not present any evidence for the existence of such satellites. The amount of substructures predicted by CDM within a galaxy size dark matter halo is too low to explain the observed anomalies in the QSO images flux ratio. Nevertheless the fluxes of QSO multiple images can be used to constrain the CDM power spectrum on small scales and test different dark matter candidates. We show that a warm dark matter scenario, with an insufficiently massive particle, fails to reproduce the observational data. Our results suggest a lower limit of few keV (~ 10) for the mass of warm dark matter candidates in the form of a sterile neutrino, in good agreement with previous results coming from Lyman- forest and Cosmic Microwave Background analysis.

Original languageEnglish (US)
Pages (from-to)186-195
Number of pages10
JournalProceedings of the International Astronomical Union
Volume3
Issue numberS244
DOIs
StatePublished - Jun 1 2007

Fingerprint

quasars
halos
dark matter
galaxies
galactic evolution
substructures
power spectra
neutrinos
anomalies
microwaves
detection
high resolution
anomaly
simulation

Keywords

  • Dark matter
  • Galaxies: halos
  • Methods: numerical

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

QSO strong gravitational lensing and the detection of dark halos. / Maccio, Andrea.

In: Proceedings of the International Astronomical Union, Vol. 3, No. S244, 01.06.2007, p. 186-195.

Research output: Contribution to journalArticle

@article{b4635ba919a943e89c83caa7c96cfe12,
title = "QSO strong gravitational lensing and the detection of dark halos",
abstract = "We present recent results concerning the possibility to detect dark satellites around galaxies using QSO strong gravitational lensing. Combining high resolution hydrodynamical simulations of galaxy formation and analytic studies we show that current QSO observations data do not present any evidence for the existence of such satellites. The amount of substructures predicted by CDM within a galaxy size dark matter halo is too low to explain the observed anomalies in the QSO images flux ratio. Nevertheless the fluxes of QSO multiple images can be used to constrain the CDM power spectrum on small scales and test different dark matter candidates. We show that a warm dark matter scenario, with an insufficiently massive particle, fails to reproduce the observational data. Our results suggest a lower limit of few keV (~ 10) for the mass of warm dark matter candidates in the form of a sterile neutrino, in good agreement with previous results coming from Lyman- forest and Cosmic Microwave Background analysis.",
keywords = "Dark matter, Galaxies: halos, Methods: numerical",
author = "Andrea Maccio",
year = "2007",
month = "6",
day = "1",
doi = "10.1017/S1743921307013981",
language = "English (US)",
volume = "3",
pages = "186--195",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S244",

}

TY - JOUR

T1 - QSO strong gravitational lensing and the detection of dark halos

AU - Maccio, Andrea

PY - 2007/6/1

Y1 - 2007/6/1

N2 - We present recent results concerning the possibility to detect dark satellites around galaxies using QSO strong gravitational lensing. Combining high resolution hydrodynamical simulations of galaxy formation and analytic studies we show that current QSO observations data do not present any evidence for the existence of such satellites. The amount of substructures predicted by CDM within a galaxy size dark matter halo is too low to explain the observed anomalies in the QSO images flux ratio. Nevertheless the fluxes of QSO multiple images can be used to constrain the CDM power spectrum on small scales and test different dark matter candidates. We show that a warm dark matter scenario, with an insufficiently massive particle, fails to reproduce the observational data. Our results suggest a lower limit of few keV (~ 10) for the mass of warm dark matter candidates in the form of a sterile neutrino, in good agreement with previous results coming from Lyman- forest and Cosmic Microwave Background analysis.

AB - We present recent results concerning the possibility to detect dark satellites around galaxies using QSO strong gravitational lensing. Combining high resolution hydrodynamical simulations of galaxy formation and analytic studies we show that current QSO observations data do not present any evidence for the existence of such satellites. The amount of substructures predicted by CDM within a galaxy size dark matter halo is too low to explain the observed anomalies in the QSO images flux ratio. Nevertheless the fluxes of QSO multiple images can be used to constrain the CDM power spectrum on small scales and test different dark matter candidates. We show that a warm dark matter scenario, with an insufficiently massive particle, fails to reproduce the observational data. Our results suggest a lower limit of few keV (~ 10) for the mass of warm dark matter candidates in the form of a sterile neutrino, in good agreement with previous results coming from Lyman- forest and Cosmic Microwave Background analysis.

KW - Dark matter

KW - Galaxies: halos

KW - Methods: numerical

UR - http://www.scopus.com/inward/record.url?scp=39449122455&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=39449122455&partnerID=8YFLogxK

U2 - 10.1017/S1743921307013981

DO - 10.1017/S1743921307013981

M3 - Article

AN - SCOPUS:39449122455

VL - 3

SP - 186

EP - 195

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S244

ER -