Observations of diffuse fluxes of cosmic neutrinos

In this contribution the current observational results for the diffuse flux of high-energy astrophysical neutrinos are reviewed. In order to understand the science implications, the measurements in different detection channels are discussed and results are compared. The discussion focuses is the energy spectrum, the flavor ratio and large scale anisotropy.Comment: Prepared for "Neutrino Astronomy - Current Status, Future Prospects" (World Scientific) Edited by: Thomas Gaisser (University of Delaware, USA), Albrecht Karle (University of Wisconsin-Madison, USA

Calculation of oscillation probabilities of atmospheric neutrinos using nuCraft

NuCraft (nucraft.hepforge.org) is an open-source Python project that calculates neutrino oscillation probabilities for neutrinos from cosmic-ray interactions in the atmosphere for their propagation through Earth. The solution is obtained by numerically solving the Schr\"odinger equation. The code supports arbitrary numbers of neutrino flavors including additional sterile neutrinos, CP violation, arbitrary mass hierarchies, matter effects with a configurable Earth model, and takes into account the production height distribution of neutrinos in the Earth's atmosphere.Comment: submitted to Computer Physics Communication

Calculation of the Cherenkov light yield from electromagnetic cascades in ice with Geant4

In this work we investigate and parameterize the amount and angular distribution of Cherenkov photons which are generated by electromagnetic cascades in water or ice. We simulate electromagnetic cascades with Geant4 for primary electrons, positrons and photons with energies ranging from 1 GeV to 10 TeV. We parameterize the total Cherenkov light yield as a function of energy, the longitudinal evolution of the Cherenkov emission along the cascade-axis and the angular distribution of photons. Furthermore, we investigate the fluctuations of the total light yield, the fluctuations in azimuth and changes of the emission with increasing age of the cascade

Effective field theory interpretation of searches for dark matter annihilation in the Sun with the IceCube Neutrino Observatory

We present a model-independent interpretation of searches for dark matter annihilation in the Sun using an effective field theory approach. We identify a set of effective operators contributing to spin-dependent scattering of dark matter with protons in the non-relativistic limit and explore simple new physics models which would give rise to such operators. Using the limits on the spin-dependent scattering cross-section set by the IceCube collaboration in their search for dark matter annihilation in the Sun, we derive limits on effective couplings and corresponding masses of mediating particles. We show that the effective field theory interpretation of the IceCube searches provides constraints on dark matter complementary to those from relic density observations and searches at the LHC. Finally, we discuss the impact of astrophysical uncertainties on our results.Comment: 16 pages, 6 figures; Added references in v

Memory-function approach to the normal-state optical properties of the Bechgaard salt (TMTSF)_2PF_6

The gauge invariant, two-component optical conductivity model, with a correlation gap structure related to the umklapp scattering processes, is applied to the quasi-one-dimensional electronic systems and compared to the recent measurements on the Bechgaard salt (TMTSF)_2PF_6. The optical response of both the insulating and metallic state is found for the half-filled conduction band, depending on the ratio between the correlation energy scale 2 \Delta^0_2 and the transfer integral in the direction perpendicular to the conducting chains, t_{{\rm b}'}. The estimated value 2 \Delta^0_2/t_{{\rm b}'} agrees reasonably well with the previous experimental and theoretical conclusions. Parallel to the chains the thermally activated conduction electrons in the insulating state are found to exhibit an universal behaviour, accounting for the observed single-particle optical conductivity of the ordered ground state of charge-density-wave systems. The band parameters and the related damping energies suitable to the normal metallic state of (TMTSF)_2PF_6 are estimated from the measured spectra. Not only the spectral weights but also the damping energies clearly indicate an opening of the correlation gap in the charge excitation spectrumComment: 11 pages, 7 figure

Diffuse Emission of Galactic High-Energy Neutrinos from a Global Fit of Cosmic Rays

In the standard picture of galactic cosmic rays, a diffuse flux of high-energy gamma-rays and neutrinos is produced from inelastic collisions of cosmic ray nuclei with the interstellar gas. The neutrino flux is a guaranteed signal for high-energy neutrino observatories such as IceCube, but has not been found yet. Experimental searches for this flux constitute an important test of the standard picture of galactic cosmic rays. Both the observation and non-observation would allow important implications for the physics of cosmic ray acceleration and transport. We present CRINGE, a new model of galactic diffuse high-energy gamma-rays and neutrinos, fitted to recent cosmic ray data from AMS-02, DAMPE, IceTop as well as KASCADE. We quantify the uncertainties for the predicted emission from the cosmic ray model, but also from the choice of source distribution, gas maps and cross-sections. We consider the possibility of a contribution from unresolved sources. Our model predictions exhibit significant deviations from older models. Our fiducial model is available at https://doi.org/10.5281/zenodo.7373010 .Comment: 30 pages, 14 figures; references adde

Afterpulse Measurements of R7081 Photomultipliers for the Double Chooz Experiment

We present the results of afterpulse measurements performed as qualification test for 473 inner detector photomultipliers of the Double Chooz experiment. The measurements include the determination of a total afterpulse occurrence probability as well as an average time distribution of these pulses. Additionally, more detailed measurements with different light sources and simultaneous charge and timing measurements were performed with a few photomultipliers to allow a more detailed understanding of the effect. The results of all measurements are presented and discussed