4.2 Article

Intrinsic neutron background of nuclear emulsions for directional Dark Matter searches

Journal

ASTROPARTICLE PHYSICS
Volume 80, Issue -, Pages 16-21

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.astropartphys.2016.03.003

Keywords

Dark matter; Neutron background; Radiopurity; Nuclear emulsions

Funding

  1. JSPS [25800140, 14429969]
  2. Grants-in-Aid for Scientific Research [13J09097, 26104005, 14J11132, 25800140, 26302003, 15J06702, 15H05446] Funding Source: KAKEN

Ask authors/readers for more resources

Recent developments of the nuclear emulsion technology led to the production of films with nanometric silver halide grains suitable to track low energy nuclear recoils with submicrometric length. This improvement opens the way to a directional Dark Matter detection, thus providing an innovative and complementary approach to the on-going WIMP searches. An important background source for these searches is represented by neutron-induced nuclear recoils that can mimic the WIMP signal. In this paper we provide an estimation of the contribution to this background from the intrinsic radioactive contamination of nuclear emulsions. We also report the neutron-induced background as a function of the read-out threshold, by using a GEANT4 simulation of the nuclear emulsion, showing that it amounts to about 0.06 per year per kilogram, fully compatible with the design of a 10 kg x year exposure. (C) 2016 Elsevier B.V. All rights reserved.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.2
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Chemistry, Inorganic & Nuclear

Monte Carlo simulation of background components in low level Germanium spectrometry

Nicola Ackermann, Hannes Bonet, Christian Buck, Oleg Chkvorets, Janina Hakenmueller, Gerd Heusser, Matthias Laubenstein, Manfred Lindner, Werner Maneschg, Jochen Schreiner, Herbert Strecker

Summary: This study presents the decomposition of the background spectra of four screening detectors GeMPI 1-4 at Gran Sasso Underground Laboratory (LNGS) using Monte Carlo simulations in the Geant4-based framework MaGe. A detailed understanding of the background spectra composition was achieved, proposing two new shield designs for future GeMPI-like detectors and reducing the integrated background count rate to 15 counts/d/kg in the energy range of [40, 2700] keV.

APPLIED RADIATION AND ISOTOPES (2023)

Article Chemistry, Analytical

A new multidisciplinary non-destructive protocol for the analysis of stony meteorites: gamma spectroscopy, neutron and muon techniques supported by Raman microscopy and SEM-EDS

Riccardo Rossini, Daniela Di Martino, Toluwalase Agoro, Matteo Cataldo, Giuseppe Gorini, Adrian D. D. Hillier, Matthias Laubenstein, Giulia Marcucci, Maya Musa, Maria Pia Riccardi, Antonella Scherillo, Massimiliano Clemenza

Summary: This study demonstrates the use of non-destructive measurements to characterize a stony meteorite. Various techniques, such as gamma ray spectrometry, Time-of-Flight Neutron Diffraction, Neutron Resonance Capture Analysis, and micro-Raman Spectroscopy, were applied to identify the sample, analyze its mineralogical phase, and study the presence and distribution of certain elements.

JOURNAL OF ANALYTICAL ATOMIC SPECTROMETRY (2023)

Article Instruments & Instrumentation

First measurements of remoTES cryogenic calorimeters: Easy-to-fabricate particle detectors for a wide choice of target materials

G. Angloher, M. R. Bharadwaj, I. Dafinei, N. Di Marco, L. Einfalt, F. Ferroni, S. Fichtinger, A. Filipponi, T. Frank, M. Friedl, A. Fuss, Z. Ge, M. Heikinheimo, K. Huitu, M. Kellermann, R. Maji, M. Mancuso, L. Pagnanini, F. Petricca, S. Pirro, F. Probst, G. Profeta, A. Puiu, F. Reindl, K. Schaffner, J. Schieck, D. Schmiedmayer, C. Schwertner, M. Stahlberg, A. Stendahl, F. Wagner, S. Yue, V. Zema, Y. Zhu, A. Bento, L. Canonica, A. Garai

Summary: Low-temperature calorimeters based on Transition Edge Sensors (TESs) are suitable for rare event searches. The novel design of the thermometer coupling, called remoTES, extends the applicability of the TES technology to a wider range of potential absorber materials, including hygroscopic and low melting point materials. Experimental results show that remoTES calorimeters achieve high energy resolution for both silicon and alpha-TeO2 absorbers. The simplified production process and higher reproducibility make remoTES calorimeters more desirable for large detector arrays.

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT (2023)

Article Physics, Multidisciplinary

Updated constraints on sterile neutrino mixing in the OPERA experiment using a new νe identification method

N. Agafonova, A. Alexandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, C. Bozza, R. Brugnera, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D'Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievsky, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, S. Gorbunov, Y. Gornushkin, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, K. Ishiguro, A. Iuliano, K. Jakovcc, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, S. Ogawa, N. Okateva, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, E. Shibayama, H. Shibuya, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, C. S. Yoon

Summary: This paper presents a novel method for identifying low-energy (less than 30 GeV) νe using an improved emulsion film scanning system. The method is expected to increase the detection efficiency of νe in the low-energy region by 25-70%, leading to enhanced sensitivity of OPERA to neutrino oscillations in the 3 + 1 model. By applying this method to a subset of data, one additional νe candidate is identified. The combined analysis with the appearance of ντ improves the upper limit on sin^2(2)θμe to 0.016 at 90% C.L. in the Mini-BooNE allowed region Δm^2 ~ 0.3 eV^2.

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS (2023)

Article Chemistry, Inorganic & Nuclear

Cosmogenic radionuclides in the Cavezzo meteorite: Gamma-ray measurement and detection efficiency simulations

Ilaria Bizzarri, Dario Barghini, Paolo Colombetti, Daniele Gardiol, Sara Rubinetti, Salvatore Mancuso, Mario Di Martino, Giovanni Pratesi, Vanni Moggi Cecchi, Nora Groschopf, Andrea Aquino, Matthias Laubenstein, Narendra Bhandari, Carla Taricco

Summary: The Cavezzo meteorite was recovered just three days after its fall over Northern Italy. It was classified as an L5 anomalous chondrite and two specimens were collected. The gamma-activity of the meteorite was measured using a large-volume HPGe-NaI(Tl) spectrometer to detect cosmogenic radioisotopes.

APPLIED RADIATION AND ISOTOPES (2023)

Article Chemistry, Inorganic & Nuclear

Secular equilibrium assessment in a CaWO4 target crystal from the dark matter experiment CRESST using Bayesian likelihood normalisation

G. Angloher, S. Banik, G. Benato, A. Bento, A. Bertolini, R. Breier, C. Bucci, J. Burkhart, L. Canonica, A. D'Addabbo, S. Di Lorenzo, L. Einfalt, A. Erb, F. v. Feilitzch, N. Ferreiro Iachellini, S. Fichtinger, D. Fuchs, A. Fuss, A. Garai, V. M. Ghete, P. Gorla, S. Gupta, D. Hauff, M. Jeskovsky, J. Jochum, M. Kaznacheeva, A. Kinast, H. Kluck, H. Kraus, A. Langenkaemper, M. Mancuso, L. Marini, V. Mokina, A. Nilima, M. Olmi, T. Ortmann, C. Pagliarone, L. Pattavina, F. Petricca, W. Potzel, P. Povinec, F. Proebst, F. Pucci, F. Reindl, J. Rothe, K. Schaeffner, J. Schieck, D. Schmiedmayer, S. Schoenert, C. Schwertner, M. Stahlberg, L. Stodolsky, C. Strandhagen, R. Strauss, I. Usherov, F. Wagner, M. Willers, V. Zema, F. Ferella, M. Laubenstein, S. Nisi

Summary: CRESST, a leading dark matter experiment, utilized cryogenic bolometers to detect nuclear recoils from the target crystal nuclei of CaWO4 during its second phase. The previously established electromagnetic background model, based on Secular Equilibrium (SE) assumptions, was validated in this study by comparing two likelihood-based normalization results using a Bayesian likelihood approach. Despite the deviations from SE observed in some cases, it was concluded that these deviations were artifacts of the fit and that the assumptions of SE are physically meaningful.

APPLIED RADIATION AND ISOTOPES (2023)

Article Physics, Multidisciplinary

A Novel Approach to Parameter Determination of the Continuous Spontaneous Localization Collapse Model

Kristian Piscicchia, Alessio Porcelli, Angelo Bassi, Massimiliano Bazzi, Mario Bragadireanu, Michael Cargnelli, Alberto Clozza, Luca De Paolis, Raffaele Del Grande, Maaneli Derakhshani, Diosi Lajos, Sandro Donadi, Carlo Guaraldo, Mihai Iliescu, Matthias Laubenstein, Simone Manti, Johann Marton, Marco Miliucci, Fabrizio Napolitano, Alessandro Scordo, Francesco Sgaramella, Diana Laura Sirghi, Florin Sirghi, Oton Vazquez Doce, Johann Zmeskal, Catalina Curceanu

Summary: Models of dynamical wave function collapse describe the breakdown of quantum superposition due to system mass increase by introducing non-linear and stochastic modifications to Schrodinger dynamics. Continuous Spontaneous Localization (CSL) has been extensively studied theoretically and experimentally. Measurable consequences of the collapse phenomenon depend on different combinations of the model parameters (strength λ and correlation length r(C)), leading to exclusion of certain regions in the parameter space (λ - r(C)).

ENTROPY (2023)

Article Multidisciplinary Sciences

Underground Tests of Quantum Mechanics by the VIP Collaboration at Gran Sasso

Fabrizio Napolitano, Andrea Addazi, Angelo Bassi, Massimiliano Bazzi, Mario Bragadireanu, Michael Cargnelli, Alberto Clozza, Luca De Paolis, Raffaele Del Grande, Maaneli Derakhshani, Sandro Donadi, Carlo Fiorini, Carlo Guaraldo, Mihail Iliescu, Matthias Laubenstein, Simone Manti, Antonino Marciano, Johann Marton, Marco Miliucci, Edoardo Milotti, Kristian Piscicchia, Alessio Porcelli, Alessandro Scordo, Francesco Sgaramella, Diana Laura Sirghi, Florin Sirghi, Oton Vazquez Doce, Johann Zmeskal, Catalina Curceanu

Summary: Modern physics builds on the success of Quantum Mechanics in describing the microscopic world, but open questions about measurement and wave function collapse remain. To explore models beyond standard QM, we conduct experiments at the Italian National Gran Sasso underground Laboratory using radiation detectors. We have excluded the natural parameterless version of the Diosi-Penrose model and set strict bounds on the CSL model. Our VIP-2 experiment aims to detect violations of the Pauli Exclusion Principle in Copper and the VIP-3 experiment upgrade is planned for the near future. We also discuss the VIP-Lead experiment and its importance in constraining non-commutative quantum gravity theories.

SYMMETRY-BASEL (2023)

Article Multidisciplinary Sciences

SND@LHC: A New Experiment in Neutrino Physics at the LHC

Antonia Di Crescenzo, Giuliana Galati, SND LHC Collaboration

Summary: The SND@LHC detector experiment aims to measure high-energy neutrinos produced at the LHC for the first time. It is designed with multiple components to differentiate interactions involving all three neutrino flavors and investigate heavy flavor production in the forward region. This research is significant for future circular colliders and high-energy astrophysical neutrino experiments.

SYMMETRY-BASEL (2023)

Article Astronomy & Astrophysics

Directional sensitivity of the NEWSdm experiment to cosmic ray boosted dark matter

N. Y. Agafonova, A. Alexandrov, A. M. Anokhina, T. Asada, V. V. Ashikhmin, D. Centanni, M. M. Chernyavskii, N. D'Ambrosio, G. De Lellis, A. Di Crescenzo, Y. C. Dowdy, S. Dmitrievski, R. I. Enikeev, G. Galati, V. I. Galkin, A. Golovatiuk, S. A. Gorbunov, Y. Gornushkin, A. M. Guler, V. V. Gulyaeva, A. Iuliano, E. V. Khalikov, S. H. Kim, N. S. Konovalova, Y. O. Krasilnikova, A. Lauria, K. Y. Lee, V. P. Loschiavo, A. K. Managadze, A. Miloi, M. C. Montesi, T. Naka, N. M. Okateva, B. D. Park, D. A. Podgrudkov, N. G. Polukhina, T. M. Roganova, G. Rosa, M. A. Samoilov, Z. T. Sadykov, K. Saeki, O. Sato, I. R. Shakiryanova, T. V. Shchedrina, T. Shiraishi, J. Y. Sohn, A. Sotnikov, N. I. Starkov, E. N. Starkova, D. M. Strekalina, V. Tioukov, E. D. Ursov, A. Ustyuzhanin, S. Vasina, R. A. Voronkov, C. S. Yoonn

Summary: This study presents a directional search for boosted Dark Matter using a module of the NEWSdm experiment. The module consists of Nano Imaging Trackers with nanometric granularity, which allows for a low background. The module is installed on an equatorial telescope and can detect an excess of nuclear recoils induced by boosted Dark Matter pointing towards the Galactic Center. The surface laboratory configuration is the most powerful approach for a directional observation with high sensitivity.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2023)

Article Instruments & Instrumentation

Analysis of test beam data taken with a prototype of TPC with resistive Micromegas for the T2K Near Detector upgrade

D. Attie, O. Ballester, M. Batkiewicz-Kwasniak, P. Billoir, A. Blanchet, A. Blondel, S. Bolognesi, R. Boullon, D. Calvet, M. P. Casado, M. G. Catanesi, M. Cicerchia, G. Cogo, P. Colas, G. Collazuol, C. Dalmazzone, T. Daret, A. Delbart, A. De Lorenzis, S. Dolanj, K. Dygnarowicz, J. Dumarchez, S. Emery-Schrenk, A. Ershova, G. Eurin, M. Feltre, C. Forza, L. Giannessi, C. Giganti, F. Gramegna, M. Grassi, M. Guigue, P. Hamacher-Baumann, S. Hassani, D. Henaff, F. Iacob, C. Jesus-Valls, S. Joshi, R. Kurjata, M. Lamoureux, A. Langella, J. F. Laporte, L. Lavitola, M. Lehuraux, A. Longhin, T. Lux, L. Magaletti, T. Marchi, L. Mellet, M. Mezzetto, L. Munteanu, Q. V. Nguyen, Y. Orain, M. Pari, J. -M. Parraud, C. Pastore, A. Pepato, E. Pierre, C. Pio Garcia, B. Popov, J. Porthault, H. Przybiliski, F. Pupilli, T. Radermacher, E. Radicioni, F. Rossi, S. Roth, S. Russo, A. Rychter, L. Scomparin, D. Smyczek, J. Steinmann, S. Suvorov, J. Swierblewski, D. Terront, N. Thamm, F. Toussenel, V. Valentino, M. Varghese, G. Vasseur, U. Virginet, U. Yevarouskaya, M. Ziembicki, M. Zito

Summary: In this paper, the performance of the prototype High Angle Time Projection Chambers (HA-TPCs) for the T2K experiment's Near Detector (ND280) upgrade is described. The prototype TPC, equipped with the first ERAM module produced for T2K, has been exposed to an electron beam at DESY to measure spatial and dE/dx resolution. The performances of the ERAM are characterized and compared with a newly developed simulation, which accurately reproduces the main features of the data and fulfills the requirements for the HA-TPCs of T2K.

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS (2023)

Article Physics, Multidisciplinary

Observation of Collider Muon Neutrinos with the SND@LHC Experiment

R. Albanese, A. Alexandrov, F. Alicante, A. Anokhina, T. Asada, C. Battilana, A. Bay, C. Betancourt, R. Biswas, A. Blanco Castro, M. Bogomilov, D. Bonacorsi, W. M. Bonivento, P. Bordalo, A. Boyarsky, S. Buontempo, M. Campanelli, T. Camporesi, V. Canale, A. Castro, D. Centanni, F. Cerutti, M. Chernyavskiy, K. -y. Choi, S. Cholak, F. Cindolo, M. Climescu, A. P. Conaboy, G. M. Dallavalle, D. Davino, P. T. de Bryas, G. De Lellis, M. De Magistris, A. De Roeck, A. De Rujula, M. De Serio, D. De Simone, A. Di Crescenzo, R. Dona, O. Durhan, F. Fabbri, F. Fedotovs, M. Ferrillo, M. Ferro-Luzzi, R. A. Fini, A. Fiorillo, R. Fresa, W. Funk, F. M. Garay Walls, A. Golovatiuk, A. Golutvin, E. Graverini, A. M. Guler, V Guliaeva, G. J. Haefeli, J. C. Helo Herrera, E. van Herwijnen, P. Iengo, S. Ilieva, A. Infantino, A. Iuliano, R. Jacobsson, C. Kamiscioglu, A. M. Kauniskangas, E. Khalikov, S. H. Kim, Y. G. Kim, G. Klioutchnikov, M. Komatsu, N. Konovalova, S. Kovalenko, S. Kuleshov, H. M. Lacker, O. Lantwin, F. Lasagni Manghi, A. Lauria, K. Y. Lee, K. S. Lee, S. Lo Meo, V. P. Loschiavo, S. Marcellini, A. Margiotta, A. Mascellani, A. Miano, A. Mikulenko, M. C. Montesi, F. L. Navarria, S. Ogawa, N. Okateva, M. Ovchynnikov, G. Paggi, B. D. Park, A. Pastore, A. Perrotta, D. Podgrudkov, N. Polukhina, A. Prota, A. Quercia, S. Ramos, A. Reghunath, T. Roganova, F. Ronchetti, T. Rovelli, O. Ruchayskiy, T. Ruf, M. Sabate Gilarte, M. Samoilov, V. Scalera, O. Schneider, G. Sekhniaidze, N. Serra, M. Shaposhnikov, V. Shevchenko, T. Shchedrina, L. Shchutska, H. Shibuya, S. Simone, G. P. Siroli, G. Sirri, G. Soares, O. J. Soto Sandoval, M. Spurio, N. Starkov, I. Timiryasov, V. Tioukov, F. Tramontano, C. Trippl, E. Ursov, A. Ustyuzhanin, G. Vankova-Kirilova, V. Verguilov, N. Viegas Guerreiro Leonardo, C. Vilela, C. Visone, R. Wanke, E. Yaman, C. Yazici, C. S. Yoon, E. Zaffaroni, J. Zamora Saa

Summary: This study reports the direct observation of muon neutrino interactions with the SND@LHC detector at the Large Hadron Collider. Using data from proton-proton collisions collected by SND@LHC in 2022, the study shows a significant evidence of muon neutrino signals.

PHYSICAL REVIEW LETTERS (2023)

Article Astronomy & Astrophysics

First Experimental Survey of a Whole Class of Non-Commutative Quantum Gravity Models in the VIP-2 Lead Underground Experiment

Kristian Piscicchia, Antonino Marciano, Andrea Addazi, Diana Laura Sirghi, Massimiliano Bazzi, Nicola Bortolotti, Mario Bragadireanu, Michael Cargnelli, Alberto Clozza, Luca De Paolis, Raffaele Del Grande, Carlo Guaraldo, Mihail Iliescu, Matthias Laubenstein, Simone Manti, Johann Marton, Marco Miliucci, Fabrizio Napolitano, Federico Nola, Alessio Porcelli, Alessandro Scordo, Francesco Sgaramella, Florin Sirghi, Oton Vazquez Doce, Johann Zmeskal, Catalina Curceanu

Summary: This study aims to establish strict constraints on a class of non-commutative spacetime scenarios as a universality class for various quantum gravity models. It examines slight violations of the Pauli exclusion principle, as predicted by these models, by searching for Pauli forbidden K-alpha and K-beta transitions in lead. By using a high atomic number target material, the energy scale of spacetime non-commutativity emergence at high atomic transition energies can be tested. As a result, this measurement provides valuable information for setting the first constraint on the triply special relativity model proposed by Kowalski-Glikman and Smolin, with the characteristic energy scale being bound to Lambda > 5.6 . 10 (-9) Planck scales.

UNIVERSE (2023)

Review Astronomy & Astrophysics

The ESSnuSB Design Study: Overview and Future Prospects

A. Alekou, E. Baussan, A. K. Bhattacharyya, N. Blaskovic Kraljevic, M. Blennow, M. Bogomilov, B. Bolling, E. Bouquerel, F. Bramati, A. Branca, O. Buchan, A. Burgman, C. J. Carlile, J. Cederkall, S. Choubey, P. Christiansen, M. Collins, E. Cristaldo Morales, L. D'Alessi, H. Danared, D. Dancila, J. P. A. M. de Andre, J. P. Delahaye, M. Dracos, I. Efthymiopoulos, T. Ekelof, M. Eshraqi, G. Fanourakis, A. Farricker, E. Fernandez-Martinez, B. Folsom, T. Fukuda, N. Gazis, B. Galnander, Th. Geralis, M. Ghosh, A. Giarnetti, G. Gokbulut, L. Halic, M. Jenssen, R. Johansson, A. Kayis Topaksu, B. Kildetoft, B. Klicek, M. Koziol, K. Krhac, L. Lacny, M. Lindroos, A. Longhin, C. Maiano, S. Marangoni, C. Marrelli, C. Martins, D. Meloni, M. Mezzetto, N. Milas, M. Oglakci, T. Ohlsson, M. Olvegard, T. Ota, M. Pari, J. Park, D. Patrzalek, G. Petkov, P. Poussot, F. Pupilli, S. Rosauro-Alcaraz, D. Saiang, J. Snamina, A. Sosa, G. Stavropoulos, M. Stipcevic, B. Szybinski, R. Tarkeshian, F. Terranova, J. Thomas, T. Tolba, E. Trachanas, R. Tsenov, G. Vankova-Kirilova, N. Vassilopoulos, E. Wildner, J. Wurtz, O. Zormpa, Y. Zou

Summary: ESSnuSB is a design study aimed at measuring CP violation in the leptonic sector at the second neutrino oscillation maximum using a powerful neutrino beam produced by the ESS linear accelerator. The reduced impact of systematic errors at the second maximum enables a highly precise measurement of the CP violating parameter. This review discusses the advantages of measurements at the second maximum, upgrades to the ESS linac, detector complexes, and the expected physics reach of the proposed ESSnuSB experiment, as well as future developments for project realization.

UNIVERSE (2023)

Article Physics, Nuclear

Environmental sub-MeV neutron measurement at the Gran Sasso surface laboratory with a super-fine-grained nuclear emulsion detector

T. Shiraishi, S. Akamatsu, T. Naka, T. Asada, G. De Lellis, V. Tioukov, G. Rosa, R. Kobayashi, N. D'Ambrosio, A. Alexandrov, O. Sato

Summary: In this study, a super-fine-grained nuclear emulsion called nano imaging tracker was used as a neutron detector to measure the sub-MeV energy spectra of environmental neutrons. By upgrading the automated scanning system, the measurement was carried out with sufficient statistics and a flux of (7.6 +/- 1.7) x 10-3 n/(cm2 s) was measured in the proton energy range of 0.25 to 1 MeV, consistent with the prediction.

PHYSICAL REVIEW C (2023)

Article Astronomy & Astrophysics

A study on performance boost of a 17 m class Cherenkov telescope with a SiPM-based camera

Cornelia Arcaro, Michele Doro, Julian Sitarek, Dominik Baack

Summary: In this report, the performance of replacing PMTs with SiPMs in a 3rd generation IACT array (using MAGIC as an example) is investigated using generalized simulations. It is found that the use of SiPMs can improve sensitivity by a factor of three at the current trigger threshold energy, and the stronger sensitivity of SiPMs in the red part of the spectrum does not affect the performance of IACTs, which is a source of background.

ASTROPARTICLE PHYSICS (2024)

Article Astronomy & Astrophysics

Forecasts analysis on varying-a theories from gravitational wave standard sirens

L. R. Colaco, R. F. L. Holanda, Rafael C. Nunes, J. E. Gonzalez

Summary: Motivated by future gravitational wave observations, this study performs forecast analysis to constrain a possible time variation of the fine structure constant a. By considering mock data from standard sirens and current observations of strong gravitational lensing systems, it is found that future standard sirens observations can also play a significant role in the search for variations of a.

ASTROPARTICLE PHYSICS (2024)

Article Astronomy & Astrophysics

Enabling kilonova science with Nancy Grace Roman Space Telescope

Igor Andreoni, Michael W. Coughlin, Alexander W. Criswell, Mattia Bulla, Andrew Toivonen, Leo P. Singer, Antonella Palmese, E. Burns, Suvi Gezari, Mansi M. Kasliwal, R. Weizmann Kiendrebeogo, Ashish Mahabal, Takashi J. Moriya, Armin Rest, Dan Scolnic, Robert A. Simcoe, Jamie Soon, Robert Stein, Tony Travouillon

Summary: Binary neutron star mergers and neutron star-black hole mergers can be detected through gravitational waves and electromagnetic radiation. Discovering kilonovae will provide valuable insights into element nucleosynthesis and nuclear matter. The unique features of the Nancy Grace Roman Space Telescope allow for the detection of gravitational wave counterparts missed by optical telescopes.

ASTROPARTICLE PHYSICS (2024)

Review Astronomy & Astrophysics

GRMHD study of accreting massive black hole binaries in astrophysical environment: A review

Federico Cattorini, Bruno Giacomazzo

Summary: This article presents recent numerical advances in the theoretical characterization of massive binary black hole (MBBH) mergers in astrophysical environments. These systems are significant sources of gravitational waves (GWs) and promising candidates for multimessenger astronomy. Coincident detection of GWs and electromagnetic (EM) signals from merging MBBHs is a leading area of study in contemporary astrophysics. The scarcity of strong predictions for EM signals before, during, and after merger poses a major challenge in observational efforts. To address this, significant theoretical work has focused on characterizing EM counterparts that accompany GW signals. Full general relativistic modeling using Einstein's field equations coupled with magnetohydrodynamics equations has been key in producing accurate EM predictions. This review explores numerical investigations into the astrophysical manifestations of MBBH mergers and their potentially observable EM signatures.

ASTROPARTICLE PHYSICS (2024)

Article Astronomy & Astrophysics

Avoiding parameter fine-tuning in mass varying neutrino models of DE?

Michael Maziashvili, Vakhtang Tsintsabadze

Summary: Coupled models of quintessence are introduced to avoid or mitigate the parameter fine-tuning problem and also should avoid the fine-tuning problem related to the initial conditions. Coupled models can explain the timescale of the coincidence between dark energy and matter energy densities, as well as the transition of dark energy dominance. Studying the mass varying neutrino model of dark energy with inverse power-law potential helps to understand its naturalness.

ASTROPARTICLE PHYSICS (2024)