BibTex format
@article{Young:2025:epjs/s11734-025-01708-7,
author = {Young, R and Yoshida, S and Xie, C and Wissel, SA and Wang, SH and Wang, MZ and Vieregg, A and Varner, GS and Eijndhoven, NV and Touart, J and Torres, J and Toscano, S and Su, SC and Shiao, YS and Seikh, MFH and Seckel, D and Salcedo-Gomez, A and Roth, J and Punsuebsay, N and Pfendner, C and Pan, Y and Oberla, E and Nozdrina, A and Novikov, A and Nichol, RJ and Nam, J and Muzio, MS and Mase, K and Luszczak, W and Liu, TC and Liu, CH and Latif, UA and Kurusu, K and Kuo, CY and Krebs, R and Kravchenko, I and Kim, MC and Kim, KC and Kelley, JL and Karle, A and Ishihara, A and Hughes, K and Huang, MH and Hoffman, KD and Harty, N and Hanson, J and Giri, P and Gaior, R and Friedman, E and Flaherty, J and DuVernois, MA and Deaconu, C and de, Vries KD and de, Kockere S and Debolt, R and Dasgupta, P and Cummings, A and Cremonesi, L and Couberly, K and Connolly, A and Clark, BA and Chen, YC and Chen, P and Bishop, A and Besson, DZ and Beatty, JJ and Archambault, S and Allison, P and Ali, S},
doi = {epjs/s11734-025-01708-7},
journal = {European Physical Journal Special Topics},
pages = {5065--5075},
title = {Askaryan Radio Array: searching for the highest energy neutrinos},
url = {http://dx.doi.org/10.1140/epjs/s11734-025-01708-7},
volume = {234},
year = {2025}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - Searches for ultra-high energy (Eν≥10 PeV) cosmogenic and astrophysical neutrinos (UHENs) have been conducted by several experiments over the last two decades. The Askaryan Radio Array (ARA), located near the geographical South Pole, was one of the first two experiments to use radio antennas sensitive to orthogonal polarizations for detection of neutrino-induced Askaryan radiation. ARA comprises five independent autonomous stations, with an additional low-threshold phased array string with station 5, which were deployed at a depth of 100–200 m over the period 2012–2018, corresponding to a total livetime of more than 27 station-years. In this article, we present a brief overview of the detector, its detection technique, and discuss a few of its major achievements with a focus on the current status of the array-wide UHEN search. We expect to produce the most sensitive results on the neutrino flux by any existing in-ice neutrino experiment below 1000 EeV energy.
AU - Young,R
AU - Yoshida,S
AU - Xie,C
AU - Wissel,SA
AU - Wang,SH
AU - Wang,MZ
AU - Vieregg,A
AU - Varner,GS
AU - Eijndhoven,NV
AU - Touart,J
AU - Torres,J
AU - Toscano,S
AU - Su,SC
AU - Shiao,YS
AU - Seikh,MFH
AU - Seckel,D
AU - Salcedo-Gomez,A
AU - Roth,J
AU - Punsuebsay,N
AU - Pfendner,C
AU - Pan,Y
AU - Oberla,E
AU - Nozdrina,A
AU - Novikov,A
AU - Nichol,RJ
AU - Nam,J
AU - Muzio,MS
AU - Mase,K
AU - Luszczak,W
AU - Liu,TC
AU - Liu,CH
AU - Latif,UA
AU - Kurusu,K
AU - Kuo,CY
AU - Krebs,R
AU - Kravchenko,I
AU - Kim,MC
AU - Kim,KC
AU - Kelley,JL
AU - Karle,A
AU - Ishihara,A
AU - Hughes,K
AU - Huang,MH
AU - Hoffman,KD
AU - Harty,N
AU - Hanson,J
AU - Giri,P
AU - Gaior,R
AU - Friedman,E
AU - Flaherty,J
AU - DuVernois,MA
AU - Deaconu,C
AU - de,Vries KD
AU - de,Kockere S
AU - Debolt,R
AU - Dasgupta,P
AU - Cummings,A
AU - Cremonesi,L
AU - Couberly,K
AU - Connolly,A
AU - Clark,BA
AU - Chen,YC
AU - Chen,P
AU - Bishop,A
AU - Besson,DZ
AU - Beatty,JJ
AU - Archambault,S
AU - Allison,P
AU - Ali,S
DO - epjs/s11734-025-01708-7
EP - 5075
PY - 2025///
SN - 1951-6355
SP - 5065
TI - Askaryan Radio Array: searching for the highest energy neutrinos
T2 - European Physical Journal Special Topics
UR - http://dx.doi.org/10.1140/epjs/s11734-025-01708-7
VL - 234
ER -