Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR

Tobias Winchen; Stijn Buitink; Jörg Hörandel; Pragati Mitra; Katharine Mulrey; Jörg Paul Rachen

doi:10.1051/epjconf/201921604010

Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR

Tobias Winchen, Stijn Buitink, Jörg Hörandel, Pragati Mitra, Katharine Mulrey, Jörg Paul Rachen

Research output: Contribution to journal › Conference paper

Abstract

The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.

Original language	English
Article number	04010
Number of pages <span style="color:red"p> <font size="1.5"> ✽ </span> </font>	3
Journal	EPJ Web of Conferences
Volume	216
DOIs	https://doi.org/10.1051/epjconf/201921604010
Publication status	Published - 24 Sep 2019
Event	The 8th international workshop on Acoustic and Radio EeV Neutrino Detection Activities - LNS-INFN, Catania, Italy Duration: 12 Jun 2018 → 15 Jun 2018 https://indico.cern.ch/event/667036/

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10.1051/epjconf/201921604010

SRP8: Strategic Research Programme: High-Energy Physics at the VUB
D'Hondt, J., Van Eijndhoven, N., Craps, B. & Buitink, S.
1/11/12 → 31/10/24
Project: Fundamental

Cite this

@article{aa1ace1016754648bd65d660cd4e5604,

title = "Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR",

abstract = "The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth{\textquoteright}s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.",

author = "Tobias Winchen and Stijn Buitink and J{\"o}rg H{\"o}randel and Pragati Mitra and Katharine Mulrey and Rachen, {J{\"o}rg Paul}",

year = "2019",

month = sep,

day = "24",

doi = "10.1051/epjconf/201921604010",

language = "English",

volume = "216",

journal = "EPJ Web of Conferences",

issn = "2101-6275",

publisher = "EDP Sciences",

note = "The 8th international workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA2018 ; Conference date: 12-06-2018 Through 15-06-2018",

url = "https://indico.cern.ch/event/667036/",

}

TY - JOUR

T1 - Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR

AU - Winchen, Tobias

AU - Buitink, Stijn

AU - Hörandel, Jörg

AU - Mitra, Pragati

AU - Mulrey, Katharine

AU - Rachen, Jörg Paul

PY - 2019/9/24

Y1 - 2019/9/24

N2 - The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.

AB - The steep decrease of the flux of ultra-high energy cosmic rays (UHECR) provides a challenge to answer the long standing question about their origin and nature. A significant increase in detector volume may be achieved byemploying Earth’s moon as a detector that is read out using existing Earth-bound radio telescopes by searching for the radio pulses emitted by the particle shower in the lunar rock. In this contribution we will report on the properties of a corresponding detection mode currently under development for the LOFAR Radio telescope.

U2 - 10.1051/epjconf/201921604010

DO - 10.1051/epjconf/201921604010

M3 - Conference paper

VL - 216

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

SN - 2101-6275

M1 - 04010

T2 - The 8th international workshop on Acoustic and Radio EeV Neutrino Detection Activities

Y2 - 12 June 2018 through 15 June 2018

ER -

Properties of the Lunar Detection Mode for ZeV-Scale Particles with LOFAR

Abstract

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Projects

SRP8: Strategic Research Programme: High-Energy Physics at the VUB

Cite this