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Statements

Subject Item
n2:RIV%2F68378271%3A_____%2F13%3A00399649%21RIV14-MSM-68378271
rdf:type
skos:Concept n18:Vysledek
dcterms:description
We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution. We derive lower bounds on the density of sources of ultra-high energy cosmic rays from the lack of significant clustering in the arrival directions of the highest energy events detected at the Pierre Auger Observatory. The density of uniformly distributed sources of equal intrinsic intensity was found to be larger than similar to (0.06 - 5) x 10(-4) Mpc(-3) at 95% CL, depending on the magnitude of the magnetic defections. Similar bounds, in the range (0.2 - 7) x 10(-4) Mpc(-3), were obtained for sources following the local matter distribution.
dcterms:title
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
skos:prefLabel
Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory Bounds on the density of sources of ultra-high energy cosmic rays from the Pierre Auger Observatory
skos:notation
RIV/68378271:_____/13:00399649!RIV14-MSM-68378271
n18:predkladatel
n19:ico%3A68378271
n3:aktivita
n12:I n12:P n12:Z
n3:aktivity
I, P(KJB100100904), P(LA08015), P(LA08016), P(LG11044), P(LG13007), P(MEB111003), P(TA01010517), Z(AV0Z10100502), Z(AV0Z10100522), Z(MSM0021620859)
n3:cisloPeriodika
5
n3:dodaniDat
n7:2014
n3:domaciTvurceVysledku
n10:8791929 n10:3028828 n10:9977449 n10:4596412 n10:8546126 n10:6549888 n10:6882323 n10:8612900 n10:9139087 n10:5113830 n10:6110630 n10:3818837 n10:5566126 n10:1038974
n3:druhVysledku
n11:J
n3:duvernostUdaju
n5:S
n3:entitaPredkladatele
n20:predkladatel
n3:idSjednocenehoVysledku
63793
n3:idVysledku
RIV/68378271:_____/13:00399649
n3:jazykVysledku
n17:eng
n3:klicovaSlova
ultra high energy cosmic rays; cosmic ray experiments
n3:klicoveSlovo
n15:ultra%20high%20energy%20cosmic%20rays n15:cosmic%20ray%20experiments
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[4DDA5102CC72]
n3:nazevZdroje
Journal of Cosmology and Astroparticle Physics
n3:obor
n6:BF
n3:pocetDomacichTvurcuVysledku
14
n3:pocetTvurcuVysledku
512
n3:projekt
n4:MEB111003 n4:LG11044 n4:LA08015 n4:LA08016 n4:KJB100100904 n4:TA01010517 n4:LG13007
n3:rokUplatneniVysledku
n7:2013
n3:svazekPeriodika
2013
n3:tvurceVysledku
Abreu, P. Nečesal, Petr Ahlers, M. Schovancová, Jaroslava Mandát, Dušan Nožka, Libor Boháčová, Martina Řídký, Jan Tománková, L. Ebr, Jan Palatka, Miroslav Chudoba, Jiří Schovánek, Petr Prouza, Michael Pech, Miroslav Aglietta, M. Vícha, Jakub Trávníček, Petr
n3:wos
000320161400011
n3:zamer
n9:MSM0021620859 n9:AV0Z10100522 n9:AV0Z10100502
s:issn
1475-7516
s:numberOfPages
20
n8:doi
10.1088/1475-7516/2013/05/009