Cutoff in the Lyman-alpha forest power spectrum: Warm IGM or warm dark matter?

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Standard

Cutoff in the Lyman-alpha forest power spectrum : Warm IGM or warm dark matter? / Garzilli, Antonella; Boyarsky, Alexey; Ruchayskiy, Oleg.

I: Physics Letters B, Bind 773, 10.10.2017, s. 258-264.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Garzilli, A, Boyarsky, A & Ruchayskiy, O 2017, 'Cutoff in the Lyman-alpha forest power spectrum: Warm IGM or warm dark matter?', Physics Letters B, bind 773, s. 258-264. https://doi.org/10.1016/j.physletb.2017.08.022

APA

Garzilli, A., Boyarsky, A., & Ruchayskiy, O. (2017). Cutoff in the Lyman-alpha forest power spectrum: Warm IGM or warm dark matter? Physics Letters B, 773, 258-264. https://doi.org/10.1016/j.physletb.2017.08.022

Vancouver

Garzilli A, Boyarsky A, Ruchayskiy O. Cutoff in the Lyman-alpha forest power spectrum: Warm IGM or warm dark matter? Physics Letters B. 2017 okt. 10;773:258-264. https://doi.org/10.1016/j.physletb.2017.08.022

Author

Garzilli, Antonella ; Boyarsky, Alexey ; Ruchayskiy, Oleg. / Cutoff in the Lyman-alpha forest power spectrum : Warm IGM or warm dark matter?. I: Physics Letters B. 2017 ; Bind 773. s. 258-264.

Bibtex

@article{ade9cabdbd2542328b7b8541e94ff9ba,
title = "Cutoff in the Lyman-alpha forest power spectrum: Warm IGM or warm dark matter?",
keywords = "Cosmology, Warm dark matter, Large scale structure of Universe, Methods, Numerical, Observational, Quasars, Absorption lines",
author = "Antonella Garzilli and Alexey Boyarsky and Oleg Ruchayskiy",
year = "2017",
month = oct,
day = "10",
doi = "10.1016/j.physletb.2017.08.022",
language = "English",
volume = "773",
pages = "258--264",
journal = "Physics Letters B: Particle Physics, Nuclear Physics and Cosmology",
issn = "0370-2693",
publisher = "Elsevier",

}

RIS

TY - JOUR

T1 - Cutoff in the Lyman-alpha forest power spectrum

T2 - Warm IGM or warm dark matter?

AU - Garzilli, Antonella

AU - Boyarsky, Alexey

AU - Ruchayskiy, Oleg

PY - 2017/10/10

Y1 - 2017/10/10

KW - Cosmology, Warm dark matter, Large scale structure of Universe

KW - Methods, Numerical, Observational

KW - Quasars, Absorption lines

U2 - 10.1016/j.physletb.2017.08.022

DO - 10.1016/j.physletb.2017.08.022

M3 - Journal article

VL - 773

SP - 258

EP - 264

JO - Physics Letters B: Particle Physics, Nuclear Physics and Cosmology

JF - Physics Letters B: Particle Physics, Nuclear Physics and Cosmology

SN - 0370-2693

ER -

ID: 185908821