0000000000305606

AUTHOR

Anna Nelles

showing 2 related works from this author

IceCube-Gen2: The Window to the Extreme Universe

2020

The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the proce…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HENuclear and High Energy PhysicsActive galactic nucleus010308 nuclear & particles physicsHigh-energy astronomyGravitational wavemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFOS: Physical sciencesCosmic ray01 natural sciencesUniverseNeutron star0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsmedia_common
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Observation of classically 'forbidden' electromagnetic wave propagation and implications for neutrino detection.

2018

Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled wi…

010504 meteorology & atmospheric sciencesWave propagationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesElectromagnetic radiationAtomicIce shelfParticle and Plasma Physics0103 physical sciencesddc:530NuclearInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)geographygeography.geographical_feature_categoryultra high energy photons and neutrinos010308 nuclear & particles physicsMolecularAstronomy and AstrophysicsNuclear & Particles PhysicsComputational physicsRay tracing (physics)Radio propagationNeutrino detectorcosmic ray experimentsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesRadio wave
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