bluuebunny/crossref_metadata_2025_split huggingface dataset:
From burial spaces to pilgrimage sites: the changing role of European cemeteries.
Authors: Pliberšek L. , Basle N. , Lebe S. S. 
Published: January 2020

Abstract

This chapter examines the role of military cemeteries and their relationship to pilgrimage and tourism. In particular, focus is given to the element of scale, with cemeteries being viewed as individual pilgrimage sites, pilgrimage destinations, or one of several cemeteries along a pilgrimage itinerary. First, the chapter discusses the role and dimensions of cemeteries as burial places, as a form of cultural heritage, and as tourist attractions. Attention is then turned to discussing cemeteries as personal pilgrimage spaces, pilgrimage centres and nodal points along a pilgrimage itinerary.
Dark tourism or pilgrimage in the museum? Considering the case of Emmett Till's casket.
Authors: Cook M. 
Published: January 2020

Abstract

This chapter first provides an overview of the historical context of the life, murder and the subsequent trial of the killers of Emmett Till (an African-American boy who was lynched in 1955). Next, discussion shifts to the controversial decisions that the Smithsonian faced in their efforts to obtain Till's casket for eventual display in the National Museum of African American History and Culture (NMAAHC). Attention is then drawn on the literature on pilgrimage and dark tourism to analyse whether this exhibit and the broader museum constitute an example of dark tourism, pilgrimage, or both. Finally, there are some thoughts on how Till's casket is of great symbolic importance in the current racial climate in the USA.
Intracourt Dialogue
Authors: Corley Pamela , Ward Artemus 
Published: January 2020

AbstractDissenting opinions are part of the ongoing constitutional dialogue among elites both inside and out of the judiciary. In order to illustrate how dissents contribute to the ongoing constitutional dialogue among elites, we examine the effect of dissents on majority opinions in the US Supreme Court. We empirically assess their operation on the contemporary Court. We find that dissents with certain characteristics are more effective than others on prompting the majority opinion to cite and discuss them. Specifically, majority opinions cite and discuss dissents that have a negative emotional tone; contain formal, logical, and hierarchical thinking; use adverbs; have a mixed ideological coalition; and cite a high number of Supreme Court precedents. These results suggest that strategic dissenters will have more in-house impact than others.
Force national standards comparison in the interamerican system of metrology (SIM), 100 kN compression
Authors: Poblete Juan Christian Villarroel , Betancur Ivan David , Dájer Espeleta stides , Savarin Alejandro 
Published: January 2020

This force comparison was performed between IDIC (Chile), INTI (Argentina) and INM (Colombia), members of the SIM region. Each laboratory used its national standard for the established measuring range. The comparison started in August 2013 and finished in December 2013. This comparison has an overlap with the force steps used in the CIPM Key Comparison CCM.F-K2.a.1, at force points 50 kN and 100 kN.

Main text

To reach the main text of this paper, click on Final Report. Note that this text is that which appears in Appendix B of the BIPM key comparison database kcdb.bipm.org/.
The final report has been peer-reviewed and approved for publication by the CCM, according to the provisions of the CIPM Mutual Recognition Arrangement (CIPM MRA).
A macrorealistic test in hybrid quantum optomechanics
Authors: Marchese Marta , McAleese Hannah , Bassi Angelo , Paternostro Mauro 
Published: January 2020

Abstract
We discuss a scheme for macrorealistic theories of the Leggett–Garg form (Leggett and Garg 1985 Phys. Rev. Lett.
54 857). Our scheme is based on a hybrid optomechanical system. It seems reasonable to test these inequalities with an optomechanical system, since in an optomechanical cavity it is possible to create non-classical states of the mirror through a projective measurement on the cavity field. We will present the protocol to generate such non-classicality for a general optomechanical cavity and after we will carry out a theoretical test for one of the possible formulations of these inequalities using a hybrid optomechanical system. Specifically, the inequality will be investigated for an harmonic oscillator coupled to a two-level system, which replaces the light field of the cavity. The aim is to reproduce, with this system, the evolution of a single spin-1/2 for which the inequality is violated; this is achievable through the conditioning of the two-level system which will be used as an ancilla.
The Dawn of Multimessenger Astronomy
Authors: Cowen D. F. 
Published: January 2020

Abstract
The realization of multimessenger astrophysics is opening up a new field of exploration of the most energetic phenomena in the universe. Astrophysical messengers associated with each of the four fundamental forces reach detectors buried deep underground or underwater, spread across wide swaths of land, and orbiting high above us in space. Recent detection of coincident real-time signals amongst these experiments heralds the birth of high-energy multimessenger astronomy and enables us to begin exploring and understanding their astrophysical sources. The Astrophysical Multimessenger Observatory Network (AMON) is currently linking multiple current and future high-energy neutrino, cosmic ray, gamma ray and gravitational wave observatories into a single virtual system, facilitating real-time coincidence searches for multimessenger astrophysical transients. AMON will generate alerts that will enable rapid follow-up of potential electromagnetic counterparts. We present the science case, design elements, partner observatories, and status of AMON.
First results from the CUORE experiment
Authors: Alduino C. , Alfonso K. , Avignone III F. T. , Azzolini O. , Bari G. , Bellini F. , Benato G. , Bersani A. , Biassoni M. , Branca A. , Brofferio C. , Bucci C. , Camacho A. , Caminata A. , Canonica L. , Cao X. G. , Capelli S. , Cappelli L. , Cardani L. , Carniti P. , Casali N. , Cassina L. , Chiesa D. , Chott N. , Clemenza M. , Copello S. , Cosmelli C. , Cremonesi O. , Creswick R. J. , Cushman J. S. , D’Addabbo A. , D’Aguanno D. , Dafinei I. , Davis C. J. , Dell’Oro S. , Deninno M. M. , Domizio S. Di , Vacri M. L. Di , Dompe V. , Drobizhev A. , Fang D. Q. , Faverzani M. , Ferri E. , Ferroni F. , Fiorini E. , Franceschi M. A. , Freedman S. J. , Fujikawa B. K. , Giachero A. , Gironi L. , Giuliani A. , Gladstone L. , Gorla P. , Gotti C. , Gutierrez T. D. , Han K. , Heeger K. M. , Hennings-Yeomans R. , Huang H. Z. , Keppel G. , Kolomensky Yu. G. , Leder A. , Ligi C. , Lim K. E. , Ma Y. G. , Marini L. , Martinez M. , Maruyama R. H. , Mei Y. , Moggi N. , Morganti S. , Nagorny S. S. , Napolitano T. , Nastasi M. , Nones C. , Norman E. B. , Novati V. , Nucciotti A. , Nutini I. , O’Donnell T. , Ouellet J. L. , Pagliarone C. E. , Pallavicini M. , Palmieri V. , Pattavina L. , Pavan M. , Pessina G. , Pira C. , Pirro S. , Pozzi S. , Previtali E. , Reindl F. , Rosenfeld C. , Rusconi C. , Sakai M. , Sangiorgio S. , Santone D. , Schmidt B. , Schmidt J. , Scielzo N. D. , Singh V. , Sisti M. , Taffarello L. , Terranova F. , Tomei C. , Vignati M. , Wagaarachchi S. L. , Wang B. S. , Wang H. W. , Welliver B. , Wilson J. , Wilson K. , Winslow L. A. , Wise T. , Zanotti L. , Zhang G. Q. , Zimmermann S. , Zucchelli S. 
Published: January 2020

Abstract
CUORE (Cryogenic Underground Observatory for Rare Events) is a ton-scale experiment aiming to the search of neutrino-less double beta decay in 130Te with a projected sensitivity on the Majorana effective mass close to the inverted hierarchy region. The CUORE detector consists of a segmented array of 988 TeO2 bolometers, organized in 19 towers and operated at a temperature of about 10 mK thanks to a custom cryogenic system which, besides the uncommon scale, observes several constraints from the radio-purity of the materials to the mechanical decoupling of the cooling systems. The successful commissioning of the CUORE cryogenic system has been completed early in 2016 and represents an outstanding achievement by itself. The installation of the detector proceeded along 2016 followed by the cooldown to base temperature at the beginning of 2017. The CUORE detector is now operational and has been taking science data since Spring 2017. With the first ~3 weeks of collected data, we present here the most stringent constraint on the 130Te half-live for the neutrino-less double beta decay.
The status of KAGRA underground cryogenic gravitational wave telescope
Authors: Akutsu T. , Ando M. , Araya A. , Aritomi N. , Asada H. , Aso Y. , Atsuta S. , Awai K. , Barton M. A. , Cannon K. , Craig K. , Creus W. , Doi K. , Eda K. , Enomoto Y. , Flaminio R. , Fujii Y. , Fujimoto M.-K. , Furuhata T. , Haino S. , Hasegawa K. , Hashino K. , Hayama K. , Hirobayashi S. , Hirose E. , Hsieh A. H. , Inoue Y. , Ioka K. , Itoh Y. , Kaji T. , Kajita T. , Kakizaki M. , Kamiizumi M. , Kambara S. , Kanda N. , Kanemura S. , Kaneyama M. , Kang G. , Kasuya J. , Kataoka Y. , Kawai N. , Kawamura S. , Kim C. , Kim H. , Kim J. , Kim Y. , Kimura N. , Kinugawa T. , Kirii S. , Kitaoka Y. , Kojima Y. , Kokeyama K. , Komori K. , Kotake K. , Kumar R. , Lee H. , Lee H. , Liu Y. , Luca N. , Majorana E. , Mano S. , Marchio M. , Matsui T. , Matsushima F. , Michimura Y. , Miyakawa O. , Miyamoto T. , Miyamoto A. , Miyo K. , Miyoki S. , Morii W. , Morisaki S. , Moriwaki Y. , Morozumi T. , Musha M. , Nagano S. , Nagano K. , Nakamura K. , Nakamura T. , Nakano H. , Nakano M. , Nakao K. , Narikawa T. , Quynh L.Nguyen , Ni W.-T. , Ochi T. , Oh J. , Oh S. , Ohashi M. , Ohishi N. , Ohkawa M. , Okutomi K. , Oohara K. , Alleano F. E.Peña , Pinto I. , Sago N. , Saijo M. , Saito Y. , Sakai K. , Sakai Y. , Sasaki Y. , Sasaki M. , Sato S. , Sato T. , Sekiguchi Y. , Seto N. , Shibata M. , Shimoda T. , Shinkai H. , Shoda A. , Somiya K. , Son E. , Suemasa A. , Suzuki T. , Suzuki T. , Tagoshi H. , Takahashi H. , Takahashi R. , Takamori A. , Takeda H. , Tanaka H. , Tanaka K. , Tanaka T. , Tatsumi D. , Tomaru T. , Tomura T. , Travasso F. , Tsubono K. , Tsuchida S. , Uchikata N. , Uchiyama T. , Uehara T. , Ueki S. , Ueno K. , Ushiba T. , van Putten M. H. P. M. , Vocca H. , Wada S. , Wakamatsu T. , Yamada T. , Yamamoto S. , Yamamoto T. , Yamamoto K. , Yamamoto A. , Yokoyama J. , Yokozawa T. , Yoon T. H. , Yuzurihara H. , Zeidler S. , Zhu Z.-H. 
Published: January 2020

Abstract
KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. It is the first km-class gravitational wave telescope constructed underground to reduce seismic noise, and the first km-class telescope to use cryogenic cooling of test masses to reduce thermal noise. The construction of the infrastructure to house the interferometer in the tunnel, and the initial phase operation of the interferometer with a simple 3-km Michelson configuration have been completed. The first cryogenic operation is expected in 2018, and the observing runs with a full interferometer are expected in 2020s. The basic interferometer configuration and the current status of KAGRA are described.
Cosmic Rays Investigation by the PAMELA experiment
Authors: Panico Beatrice , Campana D. , Osteria G. , Barbarino G. C. , Adriani O. , Bongi M. , Spillantini P. , Mori N. , Papini P. , Vannuccini E. , Bazilevskaya G. A. , Kvashnin A. N. , Stozhkov Y. I. , Bellotti R. , Monaco A. , Bruno A. , Cafagna F. , Boezio M. , Bonvicini V. , Mocchiutti E. , Munini R. , Zampa G. , Zampa N. , Vacchi A. , Bogomolov E. A. , Krutkov S. Y. , Vasilyev G. I. , Carlson P. , Pearce M. , Casolino M. , Castellini G. , De Santis C. , Marcelli L. , Mergé M. , Picozza P. , Sparvoli R. , Di Felice V. , Galper A. M. , Karelin A. V. , Koldashov S. V. , Koldobskiy S. , Yurkin Y. T. , Malakhov V. , Leonov A. , Mayorov A. G. , Mikhailov V. V. , Voronov S. A. , Martucci M. , Menn W. , Simon M. , Ricci M. , Ricciarini S. B. 
Published: January 2020

Abstract
PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) is a satellite-borne experiment. It was launched on June 15th 2006 from the Baikonur space centre on board the Russian Resurs-DK1 satellite. For about 10 years PAMELA took data, giving a fundamental contribution to the cosmic ray physics. It made high-precision measurements of the charged component of the cosmic radiation challenging the standard model of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy and in the heliosphere. PAMELA gave results on different topics on a very wide range of energy. Moreover, the long PAMELA life gives the possibility to study the variation of the proton, electron and positron spectra during the last solar minimum. The time dependence of the cosmic-ray proton and helium nuclei from the solar minimum through the following period of solar maximum activity is currently being studied. Low energy particle spectra were accurately measured also for various solar events that occurred during the PAMELA mission. In this paper a review of main PAMELA results will be reported.
Status of the Project 8 Phase II
Authors: Guigue Mathieu 
Published: January 2020

Abstract
The Project 8 collaboration aims to measure the absolute neutrino mass scale using cyclotron radiation emission spectroscopy on the beta decay of tritium. The second phase of the project will measure a continuous spectrum of molecular tritium beta decays and extract the tritium endpoint value with an eV or sub-eV scale precision. Monoenergetic electrons emitted by gaseous 83mKr atoms are used to determine the relationship between cyclotron frequency and electron energy. This study allows us to optimize both the event reconstruction algorithm and the hardware configuration, in preparation for measuring the tritium beta decay spectrum. Phase II will benefit from a gas system of krypton and tritium that will allow measurement of and offline correction for magnetic field fluctuations. We present the recent progress in understanding the electron kinematics and implementing the magnetic field calibration.
Spectral analysis for the Majorana Demonstrator experiment
Authors: Hehn L , Abgrall N , Alvis S I , Arnquist I J , Avignone III F T , Barabash A S , Barton C J , Bertrand F E , Bode T , Bradley A W , Brudanin V , Busch M , Buuck M , Caldwell T S , Chan Y-D , Christofferson C D , Chu P-H , Cuesta C , Detwiler J A , Dunagan C , Efremenko Yu , Ejiri H , Elliott S R , Gilliss T , Giovanetti G K , Green M P , Gruszko J , Guinn I S , Guiseppe V E , Haufe C R , Henning R , Hoppe E W , Howe M A , Keeter K J , Kidd M F , Konovalov S I , Kouzes R T , Lopez A M , Martin R D , Massarczyk R , Meijer S J , Mertens S , Myslik J , O’Shaughnessy C , Othman G , Pettus W , Poon A W P , Radford D C , Rager J , Reine A L , Rielage K , Robertson R G H , Ruof N W , Shanks B , Shirchenko M , Suriano A M , Tedeschi D , Trimble J E , Varner R L , Vasilyev S , Vetter K , Vorren K , White B R , Wilkerson J F , Wiseman C , Xu W , Yakushev E , Yu C-H , Yumatov V , Zhitnikov I , Zhu B X 
Published: January 2020

Abstract
The MAJORANA DEMONSTRATOR is an experiment constructed to search for neutrinoless double-beta decays in germanium-76 and to demonstrate the feasibility to deploy a ton-scale experiment in a phased and modular fashion. It consists of two modular arrays of natural and 76Ge-enriched germanium detectors totaling 44.1kg (29.7kg enriched detectors), located at the 4850’ level of the Sanford Underground Research Facility in Lead, South Dakota, USA. Data taken with this setup since summer 2015 at different construction stages of the experiment show a clear reduction of the observed background index around the ROI for 0νββ- decay search due to improvements in shielding. We discuss the statistical approaches to search for a धνββ-signal and derive the physics sensitivity for an expected exposure of 10kg· y from enriched detectors using a profile likelihood based hypothesis test in combination with toy Monte Carlo data.
Sensitive search for double electron capture on 124Xe in XMASS-I
Authors: Hiraide Katsuki 
Published: January 2020

Abstract
Double electron capture is a rare nuclear decay process in which two orbital electrons are captured simultaneously in the same nucleus. We have conducted an improved search for two-neutrino double electron capture on 124Xe and 126Xe using 800.0 days of the XMASS-I data. As a result of fitting the observed energy spectra with the expected signal and background, no significant signal is found. Therefore, we set the most stringent lower limits on their half-lives at 2.1 × 1022 years for 124Xe and 1.9 × 1022 years for 126Xe at 90% confidence level. The limits get improved by a factor of 4.5 compared to the previous result.
Latest results from NEMO-3 and commissioning status of the SuperNEMO demonstrator
Authors: Le Noblet Thibaud 
Published: January 2020

Abstract
The NEMO-3 experience was dedicated to the search for neutrinoless double beta decays (0νββ) and to the precise measurements of the two neutrino double beta decays (2νββ). The detector was installed at Laboratoire Souterrain de Modane (LSM) and investigated ββ decays among seven isotopes from 2003 to 2011. Its unique approach combining a calorimetric and a tracking measurement allows to fully reconstruct the ββ event topology with a very low background level. This feature also permits original searches such as the investigation of the hypothetical quadruple beta decay (0ν4β). Its successor, SuperNEMO, is currently under construction at LSM and will extend the sensitivity of the 0νββ search. The latest results from NEMO-3 concerning the 150Nd and 116Cd isotopes are presented as well as the installation status of the first SuperNEMO module.
The Super Kamionade Gadolinium Project
Authors: Sekiya Hiroyuki 
Published: January 2020

Abstract
Super-Kamiokande (SK) will be upgraded to Super-Kamiokande Gd (SK-Gd). This modification will enable it to identify low energy anti-neutrinos for the world’s first observation of the Diffuse Supernova Neutrino Background (DSNB). On average, there is one core-collapse supernova somewhere in the universe each second. The neutrinos emitted from all of these supernovae since the onset of stellar formation have suffused the universe. The flux of the DSNB is expected to be several tens per square centimeter per second. Theoretical models vary, but as many as five diffused supernova neutrinos per year above 10 MeV are expected to interact in SK. However, in order to separate these signals from the much more common solar and atmospheric neutrinos and other backgrounds, we need a new detection method. In 2015, the Super-Kamiokande Collaboration approved the SK-Gd project. It is the upgrade of the SK detector via the addition of water-soluble gadolinium (Gd) salt. Since then, we have been conducting many dedicated studies and developments for deploying Gd to SK.
The NEXT experiment for neutrinoless double beta decay searches
Authors: Simón A. 
Published: January 2020

Abstract
The goal of the NEXT experiment is the observation of the neutrinoless double beta decay in 136Xe using a gaseous xenon TPC with electroluminescent amplification and specialized photodetector arrays for calorimetry and tracking. After a prototyping period (2009-2014) where the technique was demonstrated, the Collaboration has completed the construction and started the operation of its first phase (NEXT-White or NEW) in the Laboratorio Subterraneo de Canfranc, in the Spanish Pyrenees, with the objectives of measuring in-situ the NEXT background model and the two-neutrino mode of the double beta decay under a radiopure regime. After running NEW, the Collaboration will operate a bigger detector, NEXT-100, which will look for the neutrinoless decay mode.
The Status of JUNO
Authors: Wang Zhimin 
Published: January 2020

Abstract
The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose underground experiment and the largest liquid scintillator (LS) detector going for neutrino mass hierarchy, precise measurement of neutrino oscillation parameters and other rare processes which include but not limited to solar neutrino, geo-neutrino, supernova neutrinos and the diffuse supernova neutrinos background. The 20” PMT system with ∼18000 high quantum efficiency phototubes, including Hamamatsu 20” and newly developed NNVT MCP 20” tubes, is the key component of JUNO experiment for better energy resolution, good detector response etc. This article reports the status of the JUNO experiment.
An overview of DarkBit, the GAMBIT dark matter module
Authors: Cornell Jonathan M. 
Published: January 2020

Abstract
In this conference paper, I give an overview of the capabilities of DarkBit, a module of the GAMBIT global fitting code that calculates a range of dark matter observables and corresponding experimental likelihood functions. Included in the code are limits from the dark matter relic density, multiple direct detection experiments, and indirect searches in gamma-rays and neutrinos. I discuss the capabilities of the code, and then present recent results of GAMBIT scans of the parameter space of the minimal supersymmetric standard model, with a focus on sensitivities of future dark matter searches to the current best fit regions.
Directional detection of Dark Matter with a nuclear emulsion based detector
Authors: Lellis Giovanni De 
Published: January 2020

Abstract
The nature of Dark Matter is one of the fundamental questions to be answered. Direct Dark Matter searches are focussed on the development, construction, and operation of detectors looking for the scattering of Weakly Interactive Massive Particles (WIMPs) with target nuclei. The measurement of the direction of WIMP-induced nuclear recoils is a challenging strategy to extend dark matter searches beyond the neutrino floor and provide an unambiguous signature of the detection of Galactic dark matter. Current directional experiments are based on the use of gas TPC whose sensitivity is strongly limited by the small achievable detector mass. NEWSdm is an innovative directional experiment proposal based on the use of a solid target made by newly developed nuclear emulsion films and read-out systems achieving a position accuracy of 10 nm.
NEWS-G, a Spherical Proportional Counter with low-Z target to search for sub-GeV Weakly Interacting Particles
Authors: Gorel Pierre 
Published: January 2020

Abstract
Despite several large-scale direct detection experiments operating worldwide, dark matter remains elusive. Not favoured by supersymmetric theories, the low Weakly Interacting Massive Particle (WIMP) mass regime (less than few GeV) has been largely ignored. The NEWS-G project builds on the experience gathered with the operation of the SEDINE detector at the Laboratoire Souterrain de Modane (France). The goal is to construct a 140cm diameter low-background Spherical Proportional Counter (SPC) capable of holding up to 10 bar of gas and to be operated at the SNOLAB underground facility (Canada). The use of low-Z target materials such as Ne, He and H, together with a strict selection of low activity materials will provide sensitivity to WIMP masses down to 0.1 GeV/c2. The detector is expected to be deployed in 2018.