Angular correlation of ultra-high energy cosmic rays with compact radio-loud quasars

Amitabh Virmani; Sibesh Bhattacharya; Pankaj Jain; Soebur Razzaque; John P. Ralston; Douglas W. Mckay

doi:10.1016/S0927-6505(01)00177-3

Angular correlation of ultra-high energy cosmic rays with compact radio-loud quasars

Amitabh Virmani
, Sibesh Bhattacharya
, Pankaj Jain
, Soebur Razzaque
, John P. Ralston
, Douglas W. Mckay

Research output: Contribution to journal › Article › peer-review

24 Citations (Scopus)

Abstract

Angular correlations of ultra-high energy cosmic rays with cosmologically distant sources may provide clues to these mysterious events. We compare cosmic ray tracks with energies above 10²⁰ eV to a compilation of radio-loud compact QSO positions. The statistical method emphasizes invariant quantities and a test of statistical independence of track and source distributions. Statistical independence is ruled out by several independent statistics at confidence levels of orders 97-99%, indicating that track directions and QSO source positions are correlated at a significant level.

Original language	English
Pages (from-to)	489-495
Number of pages	7
Journal	Astroparticle Physics
Volume	17
Issue number	4
DOIs	https://doi.org/10.1016/S0927-6505(01)00177-3
Publication status	Published - 2002
Externally published	Yes

ASJC Scopus subject areas

Astronomy and Astrophysics

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10.1016/S0927-6505(01)00177-3

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title = "Angular correlation of ultra-high energy cosmic rays with compact radio-loud quasars",

abstract = "Angular correlations of ultra-high energy cosmic rays with cosmologically distant sources may provide clues to these mysterious events. We compare cosmic ray tracks with energies above 1020 eV to a compilation of radio-loud compact QSO positions. The statistical method emphasizes invariant quantities and a test of statistical independence of track and source distributions. Statistical independence is ruled out by several independent statistics at confidence levels of orders 97-99\%, indicating that track directions and QSO source positions are correlated at a significant level.",

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T1 - Angular correlation of ultra-high energy cosmic rays with compact radio-loud quasars

AU - Virmani, Amitabh

AU - Bhattacharya, Sibesh

AU - Jain, Pankaj

AU - Razzaque, Soebur

AU - Ralston, John P.

AU - Mckay, Douglas W.

PY - 2002

Y1 - 2002

N2 - Angular correlations of ultra-high energy cosmic rays with cosmologically distant sources may provide clues to these mysterious events. We compare cosmic ray tracks with energies above 1020 eV to a compilation of radio-loud compact QSO positions. The statistical method emphasizes invariant quantities and a test of statistical independence of track and source distributions. Statistical independence is ruled out by several independent statistics at confidence levels of orders 97-99%, indicating that track directions and QSO source positions are correlated at a significant level.

AB - Angular correlations of ultra-high energy cosmic rays with cosmologically distant sources may provide clues to these mysterious events. We compare cosmic ray tracks with energies above 1020 eV to a compilation of radio-loud compact QSO positions. The statistical method emphasizes invariant quantities and a test of statistical independence of track and source distributions. Statistical independence is ruled out by several independent statistics at confidence levels of orders 97-99%, indicating that track directions and QSO source positions are correlated at a significant level.

UR - https://www.scopus.com/pages/publications/0036101338

U2 - 10.1016/S0927-6505(01)00177-3

DO - 10.1016/S0927-6505(01)00177-3

M3 - Article

AN - SCOPUS:0036101338

SN - 0927-6505

VL - 17

SP - 489

EP - 495

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 4

ER -

Angular correlation of ultra-high energy cosmic rays with compact radio-loud quasars

Abstract

ASJC Scopus subject areas

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