Galaxy clusters as probes for cosmology and dark matter

Research output: Chapter in Book/Report/Conference proceedingArticle in proceedings – Annual report year: 2019Researchpeer-review

Documents

DOI

  • Author: Battistelli, Elia Stefano

    Sapienza - Università di Roma, Italy

  • Author: Burigana, Carlo

    National Institute for Astrophysics, Italy

  • Author: De Bernardis, Paolo

    Sapienza - Università di Roma, Italy

  • Author: Kirillov, Alexander A.

    Dubna International University For Nature, Society And Man , Russian Federation

  • Author: Lima Neto, Gastao B.

    The Institute of Astronomy, Geophysics and Atmospheric Sciences, Brazil

  • Author: Masi, Silvia

    The Institute of Astronomy, Geophysics and Atmospheric Sciences, Brazil

  • Author: Nørgaard-Nielsen, Hans Ulrik

    Astrophysics and Atmospheric Physics, National Space Institute, Technical University of Denmark, Elektrovej, 2800, Kgs. Lyngby, Denmark

  • Author: Ostermann, Peter

    independent-research.org, Germany

  • Author: Roman, Matthieu

    Sorbonne Université, France

  • Author: Rosati, Piero

    Sorbonne Université, France

  • Author: Rossetti, Mariachiara

    Universitá degli Studi di Milano, Italy

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In recent years, significant progress has been made in building new galaxy clusters samples, at low and high redshifts, from wide-area surveys, particularly exploiting the Sunyaev-Zel'dovich (SZ) effect. A large effort is underway to identify and characterize these new systems with optical/NIR and X-ray facilities, thus opening new avenues to constraint cosmological models using structure growth and geometrical tests. A census of galaxy clusters sets constraints on reionization mechanisms and epochs, which need to be reconciled with recent limits on the reionization optical depth from cosmic microwave background (CMB) experiments. Future advances in SZ effect measurements will include the possibility to (unambiguously) measure directly the kinematic SZ effect, to build an even larger catalogue of galaxy clusters able to study the high redshift universe, and to make (spatially-)resolved galaxy cluster maps with even spectral capability to (spectrally-)resolve the relativistic corrections of the SZ effect.
Original languageEnglish
Title of host publicationProceedings of the Fourteenth Marcel Grossmann Meeting : On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistix Field Theories
EditorsMassimo Bianchi, Robert T Jantzen, Remo Ruffini
PublisherWorld Scientific
Publication date2018
Pages576-601
ISBN (Print)9789813226593
DOIs
Publication statusPublished - 2018
EventThe Fourteenth Marcel Grossmann Meeting - University of Rome “La Sapienza, Rome, Italy
Duration: 12 Jul 201518 Jul 2015

Conference

ConferenceThe Fourteenth Marcel Grossmann Meeting
Location University of Rome “La Sapienza
CountryItaly
CityRome
Period12/07/201518/07/2015
CitationsWeb of Science® Times Cited: No match on DOI

    Research areas

  • Background radiations, Cosmology, Dark energy, Dark matter, Galaxy clusters, Intracluster matter, Large scale structure of the universe, Microwave, Observational cosmology, Radio

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