
The Neutrino Oscillation Workshop NOW 2018 was held in Rosa Marina (Ostuni, Brindisi, Italy) from September 9th to September 16th, 2018. The meeting was organized by the Departments of Physics and by the Sections of the Istituto Nazionale di Fisica Nucleare (INFN) of Bari and Lecce, with the financial support of the Italian Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR), of the INFN, and of the Universities of Bari and Salento. For the NOW 2018 Workshop Proceedings presented hereafter, we acknowledge partial support from MIUR through the Project of Relevant National Interest n. 2017W4HA7S (PRIN) NAT-NET: Neutrino and Astroparticle Theory Network.
NOW 2018 is the tenth of a series of Workshops, the first of which (NOW 1998) was held at NIKHEF (Amsterdam) in 1998. The second to ninth workshops (NOW 2000, 2004, 2006, 2008, 2010, 2012, 2014, 2016) took place in Otranto (Lecce, Italy). For the 2018 meeting, we selected the "Ostuni Rosa Marina Resort" location in Rosa Marina (Ostuni, Italy). Further information about NOW 2018 and its previous editions can be found at the website http://www.ba.infn.it/now . NOW remains among the few, well established “Major Conference Series” in high-energy physics, which have been selected on the SPIRES-HEP conference database: http://inspirehep.net/info/Conferences/series .
The inspiring idea of the NOW series is to organize a specialized meeting three months after the International Neutrino Conference, in order to stimulate the exchange of opinions in a truly workshop-like atmosphere, with a few survey talks, short contributions, and ample time for discussion among the participants. The Workshop is focused on one of the hottest topics of contemporary physics, i.e., Neutrino Oscillations, together with its connections with particle physics, cosmic ray physics, astrophysics, and cosmology. Indeed, a growing emphasis is being given to astroparticle physics and multimessenger astronomy in the Workshop. Starting from NOW 2000, it was decided to publish the Proceedings of this series; in particular, the NOW 2000, 2004, 2006, 2008, 2010, 2012 and 2014 Proceedings appeared in Nucl. Phys. B (Proc. Suppl.), in Vols. 100, 145, 168, 188, 217, 237-238, and 265-266 respectively. The NOW 2016 Proceedings appeared as electronic version in Proceedings of Science (SISSA, Italy), available at: https://pos.sissa.it/283/ .
The structure of the NOW Workshop includes five sessions: (1) Oscillation parameters: present; (2) Oscillations parameters: future; (3) Multi-messenger astrophysics; (4) Neutrinos masses, states and interactions; (5) Particle physics in the cosmos. In the NOW 2018 poster theme, these sessions are associated to sectors of a ν Compass Rose on a hand-drawn nautical map, with the inland town being an impression of Ostuni. In each Session, one morning plenary session and two afternoon parallel sessions were dedicated to the discussion of recent results and new developments and ideas. These Proceedings can thus be considered as an up-to-date survey of the status and prospects of Neutrino Oscillation Physics (and of closely related fields in Astroparticle Physics) in 2018.
We would like to thank all the participants, a total of about 130 physicists coming from 22 different countries, and in particular the speakers and the conveners who, in collaboration with the members of the Organizing Committee, contributed with enthusiasm to the scientific success of the Workshop.
Special thanks go to all the people actively involved in the organization of the Workshop. The smooth running of the meeting was due to the invaluable work of the Administration Manager Loredana Napolitano (Bari) and of the Secretariat, formed by Daniela Dell’Anna (Lecce), Maria Concetta Gerardi (Lecce), and Antonio Silvestri (Bari), to the commitment and driving expertise of Frosino Spagna (Lecce), to the precious help of the System Manager Enrico Fasanelli and of the Technical Assistants Fulvio Ricciardi and Pierluigi Santo (Lecce). Warm thanks are also due to the PhD students Antonio De Benedittis and Margherita Di Santo for their enthusiastic collaboration in the organization.
We conclude with the hope that the eleventh workshop of the NOW series will take place in Rosa Marina in September 2020.
Organizing Committee | |
Paolo Bernardini (*) | Lecce |
Gabriella Catanesi | Bari |
Giampaolo Co’ | Lecce |
Marilisa De Serio | Bari |
Gianluigi Fogli (*) | Bari |
Francesco De Paolis | Lecce |
Eligio Lisi (*) | Bari |
Antonio Marrone | Bari |
Gennaro Miele | Napoli |
Alessandro Mirizzi | Bari |
Daniele Montanino | Lecce |
Antonio Palazzo | Bari |
Saverio Simone | Bari |
(*) Chairmen |
Scientific Advisory Committee | |
J.J. Aubert | Marseille |
J. Bernabeu | Valencia |
J. Ellis | London |
S. Hannestad | Aarhus |
C. Jarlskog | Lund |
T. Kajita | Tokyo |
S. Katsanevas | APC Paris |
P. Langacker | IAS Princeton |
M. Lindner | MPI Heidelberg |
A. McDonald | SNOLAB |
J. Panman | CERN |
G. Raffelt | Munich |
A.Yu. Smirnov | MPI Heidelberg |
Y. Suzuki | Tokyo |
J.W.F. Valle | Valencia |
R. van Dantzig | Amsterdam |
D. Vignaud | APC Paris |
S.G. Wojcicki | Stanford |
Sponsors |
Dipartimento Interateneo di Fisica “Michelangelo Merlin,” Bari |
Dipartimento di Matematica e Fisica “Ennio de Giorgi,” Lecce |
Università di Bari |
Università del Salento |
Istituto Nazionale di Fisica Nucleare (INFN) |
Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR) |
Session I: Oscillation parameters (present) |
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Neutrino Physics Results from T2K with 2.62×$10^{21}$ protons on target
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Global status of the three-neutrino mixing
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Atmospheric neutrino oscillations with IceCube
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Atmospheric neutrino oscillations with ANTARES
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Final results from OPERA
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Updated electron neutrino appearance results from MiniBooNE
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Sterile neutrino searches with the ICARUS detector
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The measurement of the pp chain solar neutrinos in Borexino
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Neutrino tomography of the earth
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T2K neutrino-nucleus cross-section results
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NA61/SHINE and EMPHATIC hadron production measurements for neutrino physics
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New results from the NUMEN project
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Oscillation Parameters Present: Session Summary
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Session II: Oscillation parameters (future) |
Neutrinos and the challenges of particle physics
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JUNO Oscillation Physics Program
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The Hyper-Kamiokande Project
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SNO+: Current Results and Future Prospects
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LiquidO: First Opaque Detector for ${\beta\beta}$ Decay?
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The design and performance of the ESS Neutrino Super Beam project ESSνSB
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The ENUBET narrow band neutrino beam
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MICE and NuStorm
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Measurements of neutrino-nucleus scattering
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The status of neutrino interaction theory and its impact on future neutrino oscillation experiments
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Systematics in T2HK, T2HKK and DUNE
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ProtoDUNE and a Dual-Phase LArTPC
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Neutrino trident production at near detectors
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Non-Unitarity vs Sterile neutrino searches
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Neutrino Oscillation Parameters: Future
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Session III: Multimessenger astrophysics |
Multi-messenger physics opportunities with core-collapse supernovae
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Distinguishing SNν equalization from a pure MSW
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Extended neutrinosphere effects on SN nu oscillations
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Galactic Cosmic Rays Anomalies
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On ultra-high energy cosmic rays
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Anisotropy studies with the Pierre Auger Observatory
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Next generation Cherenkov neutrino detectors at the South Pole
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Overview of ANTARES neutrino telescope: multimessenger results
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First results and perspectives of KM3NeT/ARCA
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Combined search of MeV ν and gravitational waves from astrophysical impulsive sources
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Multimessenger Astrophysics : Session Summary
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Session IV: Neutrino masses, states and interactions |
Light sterile neutrino oscillation searches
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Neutrinoless double beta decay: Experimental challenges
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Neutrinoless double beta decay: Theory challenges
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Status of eV-scale sterile neutrinos
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Searches for sterile neutrinos at the DANSS experiment
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SoLid: Search for oscillations with a $^6$Li detector
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Neutrinoless double beta decay search with KamLAND-Zen
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Recent results from GERDA Phase II
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CUPID-0: cryogenic calorimeters with light and heat read-out for 0νβ β searches
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First tritium results of the KATRIN analysis
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The HOLMES experiment: status and perspective
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Unbroken flavour symmetries vs lepton masses and mixings
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Magnetic moment of the neutrino
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Neutrino masses, states and interactions: session summary
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Session V: Particle Physics in the Cosmos |
Learning about Dark Matter from the Stars
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Alternative dark matter candidates: axions and ALPs
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Coherent elastic neutrino-nucleus scattering
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Dark radiation: 21cm signals and laboratory tests
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Dark neutrino interactions make gravitational waves blue
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Neutrino Oscillations and Light Dark Sectors
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Small-Scale Crisis in Cosmology – Sterile Neutrinos to the Rescue?
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Neutrino phenomenology from leptogenesis
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Leptogenesis from tiny violation of Lepton Number
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Diffuse axion-like particle searches
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CEνNS at the low-energy frontier in NU-CLEUS
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Majorons as cold light dark matter
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XENON1T results from 1 tonne×year WIMP search
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Direct detection of light WIMPs with NEWS-G
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Light dark matter investigation with CRESST
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A NaI-based cryogenic scintillating calorimeter: status and results of the COSINUS project
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Particle Physics in the Cosmos: Session Summary
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