EJErwin Jericha

Erwin Jericha

*This is an algorithmically generated author record based on publicly available information.

Current Organizations / Institutes

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Previous Organizations / Institutes

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Erwin Jericha has a total of 1000 co-authors. Here are the top co-authors by number of shared publications:


Latest Publications

  • Open Access

    Reactor operation induced thermal effects on neutron flux measurements using 3He neutron detectors at a TRIGA Mk II research reactor

    by Sebastian Dorer, Clemens Trunner, Robert Bergmann, Dieter Hainz, Erwin Jericha, Stephan Sponar, Thomas Stummer, Mario Villa

  • Open Access

    Sensitivity enhancement techniques for cryogenic calorimeters in the NUCLEUS experiment

    by M. Cappelli, A. Wallach, H. Abele, G. Angloher, B. Arnold, M. Atzori Corona, A. Bento, E. Bossio, F. Buchsteiner, J. Burkhart, et al.

    Phonon-mediated cryogenic calorimeters find application in rare event searches due to their intrinsically low energy threshold. Achieving optimal sensitivity for these kinds of detectors is crucial for signal identification, leading to various optimization techniques. In this work, we present two complementary methods to increase the sensitivity of cryogenic detectors read out by transition-edge sensors, developed and tested in the context of the NUCLEUS experiment. The first procedure maps the signal-to-noise ratio of the device across a wide range of operating points, to identify the configuration with maximal sensitivity to be used during data taking. The second method exploits the double readout of the detector, combining the information from different channels with a two-dimensional optimum filter analysis that effectively lowers the energy threshold. By combining both techniques at the same time, we obtain a baseline resolution of 2.94 ± 0.05 stat ±0.74 syst eV using a CaWO 4 based detector, achieving a promising result ahead of the first run of NUCLEUS at the experimental site.

  • Open Access

    Direct Experiments of Neutron Capture on Stable and Unstable Isotopes for Stellar Nucleosynthesis Studies

    by Jorge Lerendegui-Marco, Javier Balibrea-Correa, Victor Babiano-Suarez, César Domingo-Pardo, Gabriel de la Fuente-Rosales, Bernardo Gameiro, Ion Ladarescu, Ariel Tarifeño-Saldivia, Pablo Torres-Sánchez, Oliver Aberle, et al.

    Neutron capture reactions provide essential nuclear physics input for modeling the synthesis of heavy elements in stars. The growing precision of stellar spectroscopy and isotopic measurements in presolar SiC grains now demands cross sections with improved accuracy over the full energy range, and access to unstable nuclei relevant to slow (s-) process branchings and the intermediate (i-) process. This article reviews recent progress in direct neutron capture measurements, focusing on time-of-flight (TOF) experiments at CERN n_TOF and complementary activation techniques. Substantial advances have been achieved for stable s-only and bottleneck isotopes, significantly improving constraints on s-process models. In parallel, the combination of high instantaneous neutron fluxes and advanced detector systems has facilitated first-time neutron capture measurements on several radioactive branching-point nuclei. Feasibility studies, however, reveal current limitations related to sample availability, background conditions, and restricted energy coverage. In this context, the complementarity between TOF and activation emerges as a central strategy. Future developments, including high-flux facilities and novel inverse kinematics experiments in ion storage rings, are expected to extend the boundaries of neutron capture measurements, overcoming current limitations and helping unlock new frontiers in our understanding of stellar nucleosynthesis.

  • Open Access

    First Results of the 64Ni(n,γ) Cross Section Measurement at n_TOF

    by Michele Spelta, Gabriele Cescutti, Sergio Cristallo, Francisco García-Infantes, Alice Manna, Alberto Mengoni, Paolo Maria Milazzo, Riccardo Mucciola, Giuseppe Tagliente, Diego Vescovi, et al.

    The neutron capture cross section of 64Ni is an important parameter in nuclear astrophysics that is needed to accurately simulate stellar nucleosynthesis and validate stellar models. 64Ni is among the seeds of the s-process and its capture cross section has been found to have an important effect on the predicted abundances of many nuclei synthesized in Asymptotic Giant Branch (AGB) and massive stars. Despite its relevance, the measurements of the 64Ni(n,γ) available in the literature are scarce and discrepant. For this reason, a new accurate time-of-flight measurement has been performed at the n_TOF facility at CERN, taking advantage of its high instantaneous neutron flux, and using a highly enriched 64Ni sample. The first preliminary results show important discrepancies with respect to the cross sections recommended in the most recent releases of the evaluated nuclear data libraries. In particular, a large resonance reported at 9.52 keV is not observed. As a consequence, a significant reduction in the Maxwellian-Averaged Cross Section (MACS) obtained from evaluated data libraries in the 5–25 keV thermal energy region is expected.

  • Open Access

    Commissioning of the NUCLEUS Experiment at the Technical University of Munich

    by H. Abele, G. Angloher, B. Arnold, M. Atzori Corona, A. Bento, E. Bossio, F. Buchsteiner, J. Burkhart, F. Cappella, M. Cappelli, et al.

    The NUCLEUS experiment aims to detect coherent elastic neutrino-nucleus scattering of reactor antineutrinos on CaWO 4 targets in the fully coherent regime, using gram-scale cryogenic calorimeters. The experimental apparatus will be installed at the Chooz nuclear power plant in France, in the vicinity of two 4.25 GW th reactor cores. This work presents results from the commissioning of an essential version of the experiment at the shallow Underground Laboratory of the Technical University of Munich. For the first time, two cryogenic target detectors were tested alongside active and passive shielding systems. Over a period of two months, all detector subsystems were operated with stable performance. Background measurements were conducted, providing important benchmarks for the modeling of background sources at the reactor site. Finally, we present ongoing efforts to upgrade the detector systems in preparation for a technical run at Chooz in 2026, and highlight the remaining challenges to achieving neutrino detection.


  • Open Access

    The CRAB facility at the TU Wien TRIGA reactor: status and related physics program

    by H. Abele, P. Ajello, A. Armatol, B. Arnold, J. Billard, E. Bossio, J. Burkhart, F. Cappella, N. Casali, R. Cerulli, et al.

    The Crab (Calibrated nuclear Recoils for Accurate Bolometry) project aims to precisely characterize the response of cryogenic detectors to sub-keV nuclear recoils of direct interest for coherent neutrino-nucleus scattering and dark matter search experiments. The Crab method relies on the radiative capture of thermal neutrons in the target detector, resulting in a nuclear recoil with a well-defined energy. We present a new experimental setup installed at the TRIGA Mark-II reactor at Atominstitut (Vienna), providing a low intensity beam of thermal neutrons sent to the target cryogenic detector mounted inside a wet dilution refrigerator Kelvinox 100. After the presentation of all components of the setup we report the analysis of first commissioning data with CaWO $$_{4}$$ 4 detectors of the Nucleus experiment. They show stable operation of the cryostat and detectors on a week-scale. Due to an energy resolution currently limited to 20 eV we use neutron beam induced events at high energy, in the 10 to 100 keV range, to demonstrate the excellent agreement between the data and simulation and the accurate understanding of external background. Thanks to these data we also propose an updated decay scheme of the low-lying excited states of $$^{187}$$ 187 W. Finally, we present the first evidence of neutron-capture induced coincidences between BaF $$_2$$ 2 $$\gamma $$ γ -detectors installed around the dewar and the inner cryogenic detector. These promising results pave the way for an extensive physics program with various detector materials, like CaWO $$_{4}$$ 4 , Al $$_{2}$$ 2 O $$_{3}$$ 3 , Ge and Si.


  • Open Access

    Sub-keV Electron Recoil Calibration for Macroscopic Cryogenic Calorimeters Using a Novel X-ray Fluorescence Source

    by H. Abele, G. Angloher, B. Arnold, M. Atzori Corona, A. Bento, E. Bossio, J. Burkhart, F. Cappella, M. Cappelli, N. Casali, et al.

    Percent-level calibration of cryogenic macro-calorimeters with energy thresholds below 100 eV is crucial for light Dark Matter (DM) searches and reactor neutrino studies based on coherent elastic neutrino-nucleus scattering (CEvNS). This paper presents a novel calibration source based on X-ray fluorescence (XRF) of light elements. It uses a $$^{55}$$ 55 Fe source to irradiate a two-staged target arrangement, emitting characteristic emission lines from 677 eV to 6.5 keV. We demonstrate the potential of this new XRF source to calibrate a 0.75 g CaWO $$_4$$ 4 crystal of the NUCLEUS and CRAB experiments. Additionally, we introduce CryoLab, an advanced analysis tool for cryogenic detector data, featuring robust methods for data processing, calibration, and high-level analysis, implemented in MATLAB and HDF5. We also present a phenomenological model for energy resolution, which incorporates statistical contributions, systematic effects, and baseline noise, enabling a novel approach to evaluating athermal phonon collection efficiency in macro-calorimeters based on transition edge sensors (TES).


  • Open Access

    Decoupling pulse tube vibrations from a dry dilution refrigerator at milli-Kelvin temperatures

    by A. Wex, J. Rothe, L. Peters, H. Abele, G. Angloher, B. Arnold, M. Atzori Corona, A. Bento, E. Bossio, J. Burkhart, et al.

    With the rising adoption of dry dilution refrigerators across scientific and industrial domains, there has been a pressing demand for highly efficient vibration decoupling systems capable of operation at cryogenic temperatures in order to achieve the low vibration levels required for operation of sensitive equipment like cryogenic detectors or quantum devices. As part of the NUCLEUS experiment, a cryogenic spring pendulum has been engineered to effectively isolate pulse tube vibrations by establishing an autonomous frame of reference for the experimental volume, while sustaining temperatures below 10 mK. Attaining attenuation of up to two orders of magnitude within the region of interest of the NUCLEUS cryogenic detectors, we achieved displacement RMS values in the order of 1 nm in the axial direction and 100 pm radially, thereby reducing vibrations below typical environmental levels. Our successful detector operation across multiple cooldown cycles demonstrated negligible sensitivity to pulse tube induced vibrations, culminating in the achievement of an ultra-low (6.22 ± 0.07) eV baseline resolution on a gram-scale CaWO4 cryogenic calorimeter during continuous pulse tube operation over the course of several weeks.


  • Open Access

    A plastic scintillation muon veto for sub-Kelvin temperatures

    by A. Erhart, V. Wagner, A. Wex, C. Goupy, D. Lhuillier, E. Namuth, C. Nones, R. Rogly, V. Savu, M. Schwarz, et al.


  • Open Access

    A Plastic Scintillation Muon Veto for Sub-Kelvin Temperatures

    by A. Erhart, V. Wagner, A. Wex, C. Goupy, D. Lhuillier, E. Namuth, C. Nones, R. Rogly, V. Savu, M. Schwarz, et al.

    Rare-event search experiments located on-surface, such as short-baseline reactor neutrino experiments, are often limited by muon-induced background events. Highly efficient muon vetos are essential to reduce the detector background and to reach the sensitivity goals. We demonstrate the feasibility of deploying organic plastic scintillators at sub-Kelvin temperatures. For the NUCLEUS experiment, we developed a cryogenic muon veto equipped with wavelength shifting fibers and a silicon photo multiplier operating inside a dilution refrigerator. The achievable compactness of cryostat-internal integration is a key factor in keeping the muon rate to a minimum while maximizing coverage. The thermal and light output properties of a plastic scintillation detector were examined. We report first data on the thermal conductivity and heat capacity of the polystyrene-based scintillator UPS-923A over a wide range of temperatures extending below one Kelvin. The light output was measured down to 0.8K and observed to increase by a factor of 1.61$\pm$0.05 compared to 300K. The development of an organic plastic scintillation muon veto operating in sub-Kelvin temperature environments opens new perspectives for rare-event searches with cryogenic detectors at sites lacking substantial overburden.