Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/52631
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dc.contributor.authorAlvarez-Muniz, J.-
dc.contributor.authorJames, C.-
dc.contributor.authorProtheroe, R.-
dc.contributor.authorZas, E.-
dc.date.issued2009-
dc.identifier.citationAstroparticle Physics, 2009; 32(2):100-111-
dc.identifier.issn0927-6505-
dc.identifier.issn1873-2852-
dc.identifier.urihttp://hdl.handle.net/2440/52631-
dc.descriptionCopyright © 2009 Elsevier B.V. All rights reserved.-
dc.description.abstractThis paper presents our results for full 3-D simulations of very-high to ultra-high energy electromagnetic cascades – and the associated coherent Cherenkov radiation – as might be produced by high-energy neutrino interactions in dense media. Using “thinning” techniques, we develop an algorithm based on the existing “ZHS” code, and demonstrate that the new “ZHS-thinned” code can produce fast and accurate results for showers up to . Using ZHS-thinned, we develop new parameterisations for the radiation from showers in ice, salt, and the lunar regolith, with a separate treatment of the megaregolith (deep regolith). Our parameterisations include for the first time a method to simulate fluctuations in shower length induced by the LPM effect. Our results, which avoid the pit-falls of scaling simulations from lower energies, allow improved calculations of the detection probability for experiments searching for high-energy neutrinos using the radio technique.-
dc.description.statementofresponsibilityJ. Alvarez-Muñiz, C.W. James, R.J. Protheroe and E. Zas-
dc.language.isoen-
dc.publisherElsevier Science BV-
dc.subjectHigh-energy cosmic rays and neutrinos-
dc.subjectHigh-energy showers-
dc.subjectCherenkov radio emission-
dc.titleThinned simulations of extremely energetic showers in dense media for radio applications-
dc.typeJournal article-
dc.identifier.doi10.1016/j.astropartphys.2009.06.005-
pubs.publication-statusPublished-
Appears in Collections:Aurora harvest
Chemistry and Physics publications

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