Bibliographies thématiques / Low-energy neutrino

Littérature scientifique sur le sujet « Low-energy neutrino »

Auteur : Grafiati
Publié le 11 mars 2023

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Articles de revues sur le sujet "Low-energy neutrino"

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OBERAUER, L. « LOW ENERGY NEUTRINO PHYSICS AFTER SNO AND KamLAND ». Modern Physics Letters A 19, no 05 (20 février 2004) : 337–48. http://dx.doi.org/10.1142/s0217732304013167.

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In the recent years important discoveries in the field of low energy neutrino physics (Eν in the ≈ MeV range) have been achieved. Results of the solar neutrino experiment SNO show clearly flavor transitions from νe to νμ,τ. In addition, the long standing solar neutrino problem is basically solved. With KamLAND, an experiment measuring neutrinos emitted from nuclear reactors at large distances, evidence for neutrino oscillations has been found. The values for the oscillation parameters, amplitude and phase, have been restricted. In this paper the potential of future projects in low energy neutrino physics is discussed. This encompasses future solar and reactor experiments as well as the direct search for neutrino masses. Finally the potential of a large liquid scintillator detector in an underground laboratory for supernova neutrino detection, solar neutrino detection, and the search for proton decay p→K+ν is discussed.
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Tsakstara, V., et T. S. Kosmas. « Studying the coherent channel of neutral current ν-nucleus interaction ». HNPS Proceedings 21 (8 mars 2019) : 177. http://dx.doi.org/10.12681/hnps.2029.

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Original cross-sections calculations for neutral current neutrino scattering on 40Ar isotope are performed in the context of the quasi-particle random phase approximation (QRPA) by utilizing realistic two-nucleon forces. The incoming neutrino energy range adopted, εν ≤ 100 MeV, covers the supernova neutrinos, the low-energy beta-beam-neutrinos and the pion-muon stopped neutrino-beams existing or planned to be conducted at future neutron spallation sources. Subsequently, are the original cross sections convoluted with various supernova neutrino-energy distributions such as the two-parameter Fermi-Dirac and the power law distributions. The folded cross sections are obtained for various values of the parameters of these neutrino energy distributions corresponding to different supernova scenarios. One of the main purposes of this work is to explore the response of the 40Ar isotope as supernova neutrino detector.
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Vergados, J. D., et Y. Giomataris. « Neutral current coherent cross-sections — Implications on detecting SN and earth neutrinos with gaseous spherical TPC’s ». International Journal of Modern Physics E 26, no 01n02 (janvier 2017) : 1740030. http://dx.doi.org/10.1142/s0218301317400304.

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The detection of galactic supernova (SN) neutrinos represents one of the future frontiers of low energy neutrino physics and astrophysics. The neutron coherence of neutral currents (NCs) allows quite large cross-sections in the case of neutron rich targets, which can be exploited in detecting earth and sky neutrinos by measuring nuclear recoils. They are relatively cheap and easy to maintain. These (NC) cross-sections are not dependent on flavor conversions and, thus, their measurement will provide useful information about the neutrino source. In particular, they will yield information about the primary neutrino fluxes and perhaps about the spectrum after flavor conversions in neutrino sphere. They might also provide some clues about the neutrino mass hierarchy. The advantages of large gaseous low threshold and high resolution time projection counters (TPC) detectors are discussed.
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de Wasseige, G. « KM3NeT sensitivity to low energy astrophysical neutrinos ». Journal of Instrumentation 16, no 12 (1 décembre 2021) : C12003. http://dx.doi.org/10.1088/1748-0221/16/12/c12003.

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Abstract KM3NeT, a new generation of neutrino telescope, is currently being deployed in the Mediterranean Sea. While its two sites, ORCA and ARCA, were respectively designed for the determination of neutrino mass hierarchy and high-energy neutrino astronomy, this contribution presents a study of the detection potential of KM3NeT in the MeV-GeV energy range. At these low energies, the data rate is dominated by low-energy atmospheric muons and environmental noise due to bioluminescence and K-40 decay. The goal of this study is to characterize the environmental noise in order to optimize the selection of low-energy neutrino interactions and increase the sensitivity of KM3NeT to transient astrophysical phenomena, such as close-by core-collapse supernovae, solar flares, and extragalactic transients. In this contribution, we will study how using data science tools might improve the sensitivity of KM3NeT in these low-energy neutrino searches. We will first introduce the data sets and the different variables used to characterize KM3NeT’s response to the environmental noise. We will then compare the efficiency of various tools in identifying different components in the environmental noise and in disentangling low-energy neutrino interactions from the background events. We will conclude with the implication of low-energy neutrinos for future astrophysical transient searches.
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Bondar, Aleksandr, Alexey Buzulutskov, Aleksandr Burdakov, Evgeny Grishnyaev, Aleksandr Dolgov, Aleksandr Makarov, Sergey Polosatkin, Andrey Sokolov, Sergey Taskaev et Lev Shekhtman. « Proposal for Neutron Scattering Systems for Calibration of Dark Matter Search and Low-Energy Neutrino Detectors ». Siberian Journal of Physics 8, no 3 (1 octobre 2013) : 27–38. http://dx.doi.org/10.54362/1818-7919-2013-8-3-27-38.

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The proposal of two neutron scattering systems for calibration of two-phase cryogenic avalanche detectors with high sensitivity being developed at Budker INP is presented. This kind of detectors is designed for the search of dark matter and low energy neutrino detection, in particular, coherent neutrino scattering on nuclei. Detector calibration is made with a measurement of ionization yield and scintillation quenching factor for low energy recoiling nuclei (in 0.5 to 100 keV range) originating from elastic scattering of neutrons. To provide wide range of recoiling nuclei energies two systems of neutron scattering are proposed. The first one is based on small-sized DD generator of fast (2.45 MeV) monoenergetic neutrons operating on sealed neutron tube. The second one is based on tandem proton accelerator and lithium target and capable of generation of monoenergetic epithermal neutrons with energy up to 100 keV
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Andringa, S., J. Asaadi, J. T. C. Bezerra, F. Capozzi, D. Caratelli, F. Cavanna, E. Church et al. « Low-energy physics in neutrino LArTPCs ». Journal of Physics G : Nuclear and Particle Physics 50, no 3 (1 janvier 2023) : 033001. http://dx.doi.org/10.1088/1361-6471/acad17.

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Abstract In this paper, we review scientific opportunities and challenges related to detection and reconstruction of low-energy (less than 100 MeV) signatures in liquid argon time-projection chamber (LArTPC) neutrino detectors. LArTPC neutrino detectors designed for performing precise long-baseline oscillation measurements with GeV-scale accelerator neutrino beams also have unique sensitivity to a range of physics and astrophysics signatures via detection of event features at and below the few tens of MeV range. In addition, low-energy signatures are an integral part of GeV-scale accelerator neutrino interaction final-states, and their reconstruction can enhance the oscillation physics sensitivities of LArTPC experiments. New physics signals from accelerator and natural sources also generate diverse signatures in the low-energy range, and reconstruction of these signatures can increase the breadth of Beyond the Standard Model scenarios accessible in LArTPC-based searches. A variety of experimental and theory-related challenges remain to realizing this full range of potential benefits. Neutrino interaction cross-sections and other nuclear physics processes in argon relevant to sub-hundred-MeV LArTPC signatures are poorly understood, and improved theory and experimental measurements are needed; pion decay-at-rest sources and charged particle and neutron test beams are ideal facilities for improving this understanding. There are specific calibration needs in the low-energy range, as well as specific needs for control and understanding of radiological and cosmogenic backgrounds. Low-energy signatures, whether steady-state or part of a supernova burst or larger GeV-scale event topology, have specific triggering, DAQ and reconstruction requirements that must be addressed outside the scope of conventional GeV-scale data collection and analysis pathways. Novel concepts for future LArTPC technology that enhance low-energy capabilities should also be explored to help address these challenges.
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Sato, T. « Low energy neutrino reaction ». Nuclear Physics B - Proceedings Supplements 149 (décembre 2005) : 221–23. http://dx.doi.org/10.1016/j.nuclphysbps.2005.05.095.

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D’ANGELO, DAVIDE. « Low-energy neutrino measurements ». Pramana 79, no 4 (octobre 2012) : 757–80. http://dx.doi.org/10.1007/s12043-012-0385-3.

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Miramonti, Lino. « Neutrino Physics and Astrophysics with the JUNO Detector ». Universe 4, no 11 (16 novembre 2018) : 126. http://dx.doi.org/10.3390/universe4110126.

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The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid scintillator multi-purpose underground detector, under construction near the Chinese city of Jiangmen, with data collection expected to start in 2021. The main goal of the experiment is the neutrino mass hierarchy determination, with more than three sigma significance, and the high-precision neutrino oscillation parameter measurements, detecting electron anti-neutrinos emitted from two nearby (baseline of about 53 km) nuclear power plants. Besides, the unprecedented liquid scintillator-type detector performance in target mass, energy resolution, energy calibration precision, and low-energy threshold features a rich physics program for the detection of low-energy astrophysical neutrinos, such as galactic core-collapse supernova neutrinos, solar neutrinos, and geo-neutrinos.
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Abbasi, R., M. Ackermann, J. Adams, N. Aggarwal, J. A. Aguilar, M. Ahlers, M. Ahrens et al. « IceCube Search for Neutrinos Coincident with Gravitational Wave Events from LIGO/Virgo Run O3 ». Astrophysical Journal 944, no 1 (1 février 2023) : 80. http://dx.doi.org/10.3847/1538-4357/aca5fc.

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Abstract Using data from the IceCube Neutrino Observatory, we searched for high-energy neutrino emission from the gravitational-wave events detected by the advanced LIGO and Virgo detectors during their third observing run. We did a low-latency follow-up on the public candidate events released during the detectors’ third observing run and an archival search on the 80 confident events reported in the GWTC-2.1 and GWTC-3 catalogs. An extended search was also conducted for neutrino emission on longer timescales from neutron star containing mergers. Follow-up searches on the candidate optical counterpart of GW190521 were also conducted. We used two methods; an unbinned maximum likelihood analysis and a Bayesian analysis using astrophysical priors, both of which were previously used to search for high-energy neutrino emission from gravitational-wave events. No significant neutrino emission was observed by any analysis, and upper limits were placed on the time-integrated neutrino flux as well as the total isotropic equivalent energy emitted in high-energy neutrinos.
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Thèses sur le sujet "Low-energy neutrino"

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Allport, P. P. « High energy neutrino scattering at low Q'2 ». Thesis, University of Oxford, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.376865.

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Re, Fiorentin Michele. « Understanding and predicting low-energy neutrino parameters with leptogenesis ». Thesis, University of Southampton, 2016. https://eprints.soton.ac.uk/400882/.

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In this work, we address two major problems of the Standard Model of particle physics: the baryon asymmetry of the Universe and neutrino masses and mixing. A strict link between these two aspects can be established by the seesaw mechanism and leptogenesis. This connection can be fruitfully exploited to gain information on neutrino parameters. To this aim, we first introduce the type-I seesaw mechanism and leptogenesis, moving then to the strong thermal leptogenesis scenario. Here a large pre-existing asymmetry is efficiently erased by leptogenesis, and an analytical lower bound on the absolute neutrino mass scale can be derived. We then consider SO(10)-inspired leptogenesis, in which a set of conditions kindred to those realised in SO(10) Grand Unification Theories is imposed on the seesaw setup. A rigorous analytical study of this scenario is performed, allowing us to obtain analytical explanations of the numerous predictions on neutrino parameters. SO(10)-inspired and strong thermal SO(10)-inspired leptogenesis appear then to represent a very interesting scenario, rich of definite predictions on neutrino parameters that will be in the reach of forthcoming experiments. Finally, we examine the supersymmetric extension of SO(10)-inspired leptogenesis, analysing how the constraints on neutrino parameters change. The lower bound imposed by thermal leptogenesis on the reheating temperature is carefully studied, in light of the gravitino problem. We conclude that the thermal leptogenesis scenario represents an intriguing and viable mechanism also in the supersymmetric framework.
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Li, Tracey Chuiyee. « Phenomenology of a low-energy neutrino factory and related experiments ». Thesis, Durham University, 2010. http://etheses.dur.ac.uk/613/.

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The discovery of neutrino oscillations is one of the most important in the recent history of particle physics, being the first evidence of physics beyond the Standard Model. We describe the theoretical framework of the neutrino oscillation model, motivate the necessity for a new generation of neutrino oscillation experiments and study the phenomenological factors which influence the design of these experiments. We perform the first detailed study of a European super-beam setup using the CERN to Pyhasalmi baseline of 2285 km, analysing the physics reach of this setup with a 100 kiloton liquid argon detector and comparing its performance to that of a 50 kiloton liquid scintillator detector and a 440 kiloton water Cerenkov detector. The liquid argon and liquid scintillator detectors are found to perform best, providing sensitivity to θ₁₃, δ and the mass hierarchy for sin²2θ₁₃ > 10⁻². A potential successor to super-beam experiments is a neutrino factory. We study a low-energy neutrino factory, a setup which has so far not been analysed in any detail, performing optimisation studies and an analysis of its sensitivity to oscillation parameters and non-standard matter interactions. We show that for sin²2θ₁₃ > 4x10⁻³, a low-energy neutrino factory using a 20 kiloton totally active scintillating detector has 100% CP coverage for hierarchy sensitivity and θ₁₃ discovery, and has greater sensitivity to CP violation than the high-energy neutrino factory. We consider the novel concept of including the 'platinum channels' in addition to the 'golden channels', showing that this is a powerful way of resolving the degeneracies between the oscillation and non-standard parameters. This enhances the sensitivity, such that the low-energy neutrino factory can put upper bounds ≳10⁻² on the non-standard interaction parameters ε_eμ and ε_eτ.
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Marzola, Luca. « On leptogenesis, flavour effects and the low energy neutrino parameters ». Thesis, University of Southampton, 2012. https://eprints.soton.ac.uk/346819/.

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Contemporary physics is testing the boundaries of one of its existent paradigms, the Standard Model of Particle Physics. In recent years many attempts have been made in order to overcome the difficulties arising within this well known framework. Along with the effort made on the experimental side, for example the search for the Higgs boson at the Large Hadron Collider, there is a present requirement for testable theoretical scenarios describing physics beyond the current paradigms. To this purpose we consider the type I Seesaw extension of the Standard Model, in which the neutrino mass puzzle is possibly solved and the baryon asymmetry of the Universe explained via Leptogenesis. After reviewing the basis of the Seesaw mechanism and its recent developments we present a rigorous investigation which confirms the validity of the adopted description. Encouraged by this success we then employ the interplay of light and heavy neutrino flavour e↵ects to address the problem of initial conditions in Leptogenesis. Our analysis identifies the ⌧ N2-dominated scenario as the only possible answer, proposing a well defined setup in which successful strong thermal Leptogenesis is achieved. Attracted by the properties of our solution we consequently investigate its compatibility with the SO(10)-inspired model of Leptogenesis. The result is indeed intriguing: the strong thermal solutions of the SO(10)-inspired model deliver sharp predictions on the lowenergy neutrino parameters that fall within the reach of future neutrino experiments,opening up the possibility of a full test of this attractive Leptogenesis scenario.
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PICCIAU, EMMANUELE. « Low-energy signatures in DarkSide-50 experiment and neutrino scattering processes ». Doctoral thesis, Università degli Studi di Cagliari, 2022. http://hdl.handle.net/11584/327520.

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Dark matter is one of the greatest unsolved mysteries in cosmology nowadays. About 80% of the gravitating matter in the Universe is non-luminous, and its nature and distribution are for the most part unknown. Many experiments around the world and in space are trying to discover dark matter interactions and properties. Among them, the DarkSide project aims to see dark matter signatures inside of time projection chamber filled with liquid argon. In order to reach such a goal, the detector features along with the background must be studied and well understood. This thesis presents the so-called single-electron background of DarkSide-50 experiment, with the perspective of informing the community on the backgrounds which may affect future experiments, especially those looking for low-mass dark matter particles. Another important and irreducible background to be considered in the future regards the coherent neutrino-nucleus scattering in the detector. This process is supposed to mimic in a very similar way the dark matter interaction, making its discovery even harder. For this reason, it is crucial to increase the knowledge of the electroweak and nuclear parameters which are involved in the neutrino scattering process. In this thesis, several phenomenological studies regarding the recent discovery of coherent neutrino-nucleus scattering are presented, along with the determination of quantities accessible through this channel.
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O'Keeffe, Helen Mary. « Low energy background in the NCD phase of the Sudbury Neutrino Observatory ». Thesis, University of Oxford, 2008. http://ora.ox.ac.uk/objects/uuid:b53c04b1-5dba-4cfb-98ec-c0d8b87fb58b.

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The Sudbury Neutrino Observatory (SNO) was a 1 kilotonne heavy water Č{C}erenkov detector. Evidence for flavour changing neutrino oscillations was found by comparing the rate of Charged Current interactions with that of Neutral Current (NC) interactions. This thesis is concerned with the accurate determination of the NC flux in the Neutral Current Detector (NCD) phase of SNO. The measurement and understanding of radioactive backgrounds arising from decays of naturally occurring $^{232}$Th and $^{238}$U chain nuclei is crucial. This is because their daughter nuclei can produce neutrons via photodisintegration of deuterium. These would be indistinguishable from those produced by NC neutrino interactions. As the probability of neutron production was dependent upon the nature and location of activity, each contribution had to be determined separately. Of particular concern were $^{232}$Th and $^{238}$U in the D$_2$O and Neutral Current Detectors (NCDs). A maximum likelihood method was developed that exploited differences in the event isotropy and radial profile of each event class. These results were in agreement with water assay results and pre-deployment radioassays of the NCDs. An independent measurement of the $^{232}$Th content in the D$_2$O and H$_2$O was made by regularly assaying the water using filters loaded with hydrous titanium oxide. The concentration of $^{232}$Th in the water was determined by coincidence counting of the final assay sample. A new counter system was designed and built and the calibration and use of this system are presented. Two areas of increased activity were discovered on two of the NCDs deployed in the detector which would have prevented an accurate measurement of the NC flux. A method was devised to determine the composition and activity of one of these hotspots. The results were in good agreement with two independent methods and the uncertainty on the NC flux was reduced from $>7$% to $<1$%. The total number of neutrons produced per day by photodisintegration for $^{232}$Th and $^{238}$U in the D$_2$O and NCDs was measured to be $0.66^{+0.08}_{-0.07}$. This was significantly less than the expected 12.6 NC neutrino interactions per day. In the third phase, two independent data streams existed: PMT and NCD. A Monte Carlo study was undertaken to determine whether an accurate measure of the NC flux could be obtained using only PMT data. Results showed that no improvement could be made upon results from previous phases and the best measurement of the NC flux in the final phase would be made using PMT and NCD data.
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Manecki, Szymon M. « Annual Modulation Measurement of the Low Energy Solar Neutrino Flux with the Borexino Detector ». Diss., Virginia Tech, 2013. http://hdl.handle.net/10919/23250.

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This work reports a first attempt to measure the solar neutrino annual
flux modulation due to Earth\'s elliptical orbit with the Borexino detector. Borexino is a real-time calorimetric detector for low energy neutrino spectroscopy located in the underground laboratory of Gran Sasso, Italy. The experiment\'s main focus is the direct measurement of the 7Be solar neutrino flux of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. The original goal of this work was to quantify sensitivity of the Borexino detector to a 7% peak-to-peak signal variation over the course of a year and study background stability. A Monte-Carlo simulated sample of the expected variation was prepared in two phases of data acquisition, Phase I that spans from May-2007 to May-2010 and Phase II from October-2011 to September-2012. The data was then fitted in the time domain with a sinusoidal function and analyzed with the Lomb-Scargle fast Fourier transformation in the search for significant periodicities between periods of 0.5 and 1.5 years. The search was performed in the energy window dominated by 7Be, [210; 760] keV, and 60-day bins in the case of the fit and 10-bins for the Lomb-Scargle scan. This work also contains study of the post-purification data of Phase II beyond September-2012 with a prediction for the future sensitivity and justification of the achieved background levels.
Ph. D.
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Bilmis, Selcuk. « Study On Non Standard Interaction Of Neutrino And Unparticle Physics With Neutrino-electron Scattering Data At Low Energy In Texono Experiment ». Master's thesis, METU, 2010. http://etd.lib.metu.edu.tr/upload/12612495/index.pdf.

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Neutrino-electron scatterings are purely leptonic processes with robust Standard Model (SM) predictions. Their measurements can therefore provide constraints to physics beyond SM. The &nu
e &minus
e&minus
data taken at the Kuo-Sheng Reactor Neutrino Laboratory were used to probe two sceneria: Non-Standard Neutrino Interactions (NSI) and Unparticle Physics. New constraints were placed to the NSI parameters (&epsilon
eL , &epsilon
eR ), (&epsilon
eL , &epsilon
eR ) and (&epsilon
eL , &epsilon
eR ) , as well as to the coupling constants for scalar (&lambda
0 ) and vector (&lambda
1 ) unparticles to the neutrinos and electrons.
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Xu, Yu [Verfasser], Livia [Akademischer Betreuer] Ludhová et Achim [Akademischer Betreuer] Stahl. « Machine learning application in low energy liquid scintillator neutrino experiment / Yu Xu ; Livia Ludhová, Achim Stahl ». Aachen : Universitätsbibliothek der RWTH Aachen, 2020. http://d-nb.info/1226218601/34.

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Marta, Michele. « The 14N(p,γ)15O reaction studied at low and high beam energy ». Doctoral thesis, Saechsische Landesbibliothek- Staats- und Universitaetsbibliothek Dresden, 2012. http://nbn-resolving.de/urn:nbn:de:bsz:14-qucosa-87464.

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The CNO cycle consists of a set of nuclear reactions that convert hydrogen into helium and releases energy in stars. The cycle contributes less than 1% to our Sun's luminosity, but it is responsible for detectable neutrino fluxes that can bring direct information of the physical conditions in the solar core, provided that the nuclear reaction rate is known with sufficient precision. The 14N(p,γ)15O is the slowest reaction in the CNO cycle and estabilishes its rate. The experimental study has been performed both at the LUNA 400 kV accelerator deep underground in the Gran Sasso mountain in Italy and at a 3 MV Tandetron in the Helmholtz-Zentrum Dresden-Rossendorf. A proton beam was sent on solid TiN targets and the prompt photons were collected by a composite HPGe detector (at LUNA) or by up to four HPGe detectors (Dresden). The obtained results improve the fit of the excitation function in the R-matrix framework, that is used to extrapolate the S-factor at the very low astrophysical energies. In addition, the strength of two resonances at Ep = 430 and 897 keV of the 15N(p,αγ)12C reaction were measured, improving the precision for hydrogen depth profiling.
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Livres sur le sujet "Low-energy neutrino"

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1938-, Barger V., et Cline D. 1933-, dir. Neutrino mass and low energy weak interactions, Telemark, 1984. Singapore : World Scientific, 1985.

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Y, Suzuki, Nakahata M et Moriyama S, dir. The 2nd International Workshop on Low Energy Solar Neutrino Detection : Tokyo, Japan, 4-5 December 2000. River Edge, N.J : World Scientific, 2001.

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3

Singleterry, Robert C. Materials for low-energy neutron radiation shielding. Hampton, Va : National Aeronautics and Space Administration, Langley Research Center, 2000.

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Schopper, H., dir. Low Energy Neutrons and their Interaction with Nuclei and Matter. Part 1. Berlin/Heidelberg : Springer-Verlag, 2000. http://dx.doi.org/10.1007/b56763.

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Schopper, H., dir. Low Energy Neutrons and their Interaction with Nuclei and Matter. Part 2. Berlin/Heidelberg : Springer-Verlag, 2000. http://dx.doi.org/10.1007/b59529.

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Center, Langley Research, dir. Development of deterministic transport methods for low energy neutrons for shielding in space. Tucson, Ariz : Engineering Experiment Station, College of Engineering and Mines, University of Arizona, 1993.

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K, Nishiizumi, et United States. National Aeronautics and Space Administration., dir. Depth profile of ⁴¹Ca in an Apollo 15 drill core and the low-energy neutron flux in the moon. [New York] : Elsevier, 1997.

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8

Barger, Vernon. Neutrino Mass and Low Energy Weak Interactions. World Scientific Pub Co Inc, 1986.

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9

Suzuki, Y., M. Nakahata et S. Moriyama. Low Energy Solar Neutrino Detection : Proceedings of the 2nd International Workshop Held in Tokyo Japan 4 - 5 December 2000. World Scientific Publishing Company, 2002.

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(Contributor), T. S. Belanova, A. I. Blokhin (Contributor), A. V. Ignatyuk (Contributor), V. N. Manokhin (Contributor), A. B. Pashchenko (Contributor) et V. I. Plyaskin (Contributor), dir. Low Energy Neutron Physics (Landolt-Bornstein). Springer, 2001.

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Chapitres de livres sur le sujet "Low-energy neutrino"

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Baldo-Ceolin, Milla. « Neutrino Masses and Mixing from Neutrino Oscillations ». Dans Fundamental Interactions in Low-Energy Systems, 157–74. Boston, MA : Springer US, 1985. http://dx.doi.org/10.1007/978-1-4684-4967-9_9.

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Vitale, S., G. Darbo, G. Gallinaro, S. Siri et A. Barone. « New Detectors and Neutrino Mass ». Dans Fundamental Interactions in Low-Energy Systems, 429–34. Boston, MA : Springer US, 1985. http://dx.doi.org/10.1007/978-1-4684-4967-9_28.

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Spurio, Maurizio. « Low-Energy Neutrino Physics and Astrophysics ». Dans Astronomy and Astrophysics Library, 441–88. Cham : Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-96854-4_12.

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Zuber, Kai. « Search for the Neutrino Mass and Low Energy Neutrino Astronomy ». Dans From Ultra Rays to Astroparticles, 187–213. Dordrecht : Springer Netherlands, 2012. http://dx.doi.org/10.1007/978-94-007-5422-5_7.

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Honda, Morihiro. « Calculation of Low-Energy Atmospheric Neutrino Fluxes ». Dans Physics and Astrophysics of Neutrinos, 606–24. Tokyo : Springer Japan, 1994. http://dx.doi.org/10.1007/978-4-431-67029-2_8.

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Aglietta, M., G. Badino, G. F. Bologna, C. Castagnoli, A. Castellina, W. Fulgione, P. Galeotti et al. « Low Energy Neutrino Detection with the Mont Blanc LSD Experiment ». Dans Weak and Electromagnetic Interactions in Nuclei, 741–44. Berlin, Heidelberg : Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_144.

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Hieronymus, Maicon, Bertil Schmidt et Sebastian Böser. « Reconstruction of Low Energy Neutrino Events with GPUs at IceCube ». Dans Lecture Notes in Computer Science, 118–31. Cham : Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-50371-0_9.

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Fent, J., P. Freund, J. Gebauer, K. Pretzl, N. Schmitz, A. Singsaas, L. Stodolsky et G. Vesztergombi. « Investigation of Superconducting Tin Granules for a Low-Energy Neutrino or Dark Matter Detector ». Dans Low Temperature Detectors for Neutrinos and Dark Matter, 30–36. Berlin, Heidelberg : Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/978-3-642-72959-1_3.

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Guyot, C. « Accelerator Studies of Neutrino Oscillations : First Results from a Low-Energy Experiment at CERN ». Dans Perspectives in Particles and Fields, 519–32. Boston, MA : Springer US, 1985. http://dx.doi.org/10.1007/978-1-4757-0369-6_11.

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Wasson, O. A. « Progress in the Detection of Low-Energy Neutrons ». Dans Neutron Induced Reactions, 399–411. Dordrecht : Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4636-1_42.

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Actes de conférences sur le sujet "Low-energy neutrino"

1

Ranucci, G. « Low-Energy Neutrino Experiments (Solar Neutrinos) ». Dans The 28th International Symposium on Lepton Photon Interactions at High Energies. WORLD SCIENTIFIC, 2020. http://dx.doi.org/10.1142/9789811207402_0007.

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Bross, Alan, Malcolm Ellis, Steve Geer, Olga Mena, Silvia Pascoli, Osamu Yasuda, Naba Mondal et Chihiro Ohmori. « The Low-Energy Neutrino Factory ». Dans NEUTRINO FACTORIES, SUPERBEAMS AND BETABEAMS : 9th International Workshop on Neutrino Factories, Superbeams, and Betabeams. AIP, 2008. http://dx.doi.org/10.1063/1.2898927.

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Walter, C. W. « Low Energy Neutrino-Nucleus Interactions ». Dans NEUTRINO FACTORIES AND SUPERBEAMS : 5th International Workshop on Neutrino Factories and Superbeams ; NuFact 03. AIP, 2004. http://dx.doi.org/10.1063/1.1818408.

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Zeller, G. P. « Low Energy Neutrino Cross Sections ». Dans NEUTRINO FACTORIES AND SUPERBEAMS : 5th International Workshop on Neutrino Factories and Superbeams ; NuFact 03. AIP, 2004. http://dx.doi.org/10.1063/1.1818438.

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Bross, Alan, Malcolm Ellis, Enrique Fernández Martínez, Steve Geer, Tracey Li, Olga Mena, Silvia Pascoli, Daniel Kaplan, Maury Goodman et Zack Sullivan. « The Low Energy Neutrino Factory ». Dans NEUTRINO FACTORIES, SUPERBEAMS, AND BETA BEAMS : 11th International Workshop on Neutrino Factories, Superbeams and Beta Beams—NuFact09. AIP, 2010. http://dx.doi.org/10.1063/1.3399403.

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Hawker, E. A. « Neutrino Interactions at Low Energy ». Dans INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS : 8th Conference CIPANP2003. AIP, 2004. http://dx.doi.org/10.1063/1.1664243.

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Suzuki, Toshio. « Very low-energy neutrino interactions ». Dans INTERNATIONAL CONFERENCE ON MATHEMATICS, ENGINEERING AND INDUSTRIAL APPLICATIONS 2014 (ICoMEIA 2014). AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4919503.

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Rothe, Joannes. « CEνNS at the low-energy frontier in NU-CLEUS ». Dans Neutrino Oscillation Workshop. Trieste, Italy : Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0092.

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Jachowicz, N., et V. Pandey. « Low-energy neutrino-nucleus interactions and beta-beam neutrino ». Dans INTERNATIONAL CONFERENCE ON MATHEMATICS, ENGINEERING AND INDUSTRIAL APPLICATIONS 2014 (ICoMEIA 2014). AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4919478.

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Gaisser, T. K., et Todor Stanev. « Atmospheric neutrino fluxes at low energy ». Dans AIP Conference Proceedings Vol.126. AIP, 1985. http://dx.doi.org/10.1063/1.35157.

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Rapports d'organisations sur le sujet "Low-energy neutrino"

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Caratelli, D. Low-Energy Physics in Neutrino LArTPCs. Office of Scientific and Technical Information (OSTI), mars 2022. http://dx.doi.org/10.2172/1861356.

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Berg J. S. Options for Production Staging for a Low Energy Neutrino Factory. Office of Scientific and Technical Information (OSTI), octobre 2011. http://dx.doi.org/10.2172/1043339.

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BISHAI, M., J. HEIM, C. LEWIS, A. D. MARINO, B. VIREN et F. YUMICEVA. SIMULATION OF A WIDE-BAND LOW-ENERGY NEUTRINO BEAM FOR VERY LONG BASELINE NEUTRINO OSCILLATION EXPERIMENTS. Office of Scientific and Technical Information (OSTI), août 2006. http://dx.doi.org/10.2172/891295.

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Kyberd, Paul, Malcolm Ellis, Alan Bross, Steve Geer, Olga Mena, Ken Long, Silvia Pascoli, Enrique Fernandez Martinez, Kirk McDonald et Patrick Huber. Study of low-energy neutrino factory at the Fermilab to DUSEL baseline. Office of Scientific and Technical Information (OSTI), juillet 2009. http://dx.doi.org/10.2172/963438.

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Bishai, M., M. Diwan, S. Kettell, J. Stewart, B. Viren, E. Worcester, R. Tschirhart et L. Whitehead. Precision Neutrino Oscillation Measurements using Simultaneous High-Power, Low-Energy Project-X Beams. Office of Scientific and Technical Information (OSTI), juillet 2013. http://dx.doi.org/10.2172/1345658.

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Lenardo, B. G. Measurements and Modeling of Low Energy Nuclear Recoils in Liquid Xenon for Dark Matter and Neutrino Detection. Office of Scientific and Technical Information (OSTI), mars 2018. http://dx.doi.org/10.2172/1598951.

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Gollapinni, Sowjanya, Robert Fine et MicroBooNE et al. Search for Neutrino-Induced Neutral Current Delta Radiative Decay in MicroBooNE and a First Test of the MiniBooNE Low Energy Excess Under a Single Photon Hypothesis (submitted to PRL). Office of Scientific and Technical Information (OSTI), octobre 2021. http://dx.doi.org/10.2172/1828699.

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Lee, D. M. Low-energy neutron shielding. Office of Scientific and Technical Information (OSTI), août 1986. http://dx.doi.org/10.2172/5170723.

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Crawford, Christopher B. Precision Measurements with Low Energy Neutrons. Office of Scientific and Technical Information (OSTI), décembre 2018. http://dx.doi.org/10.2172/1487431.

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Nieschmidt, E. B. The production of low-energy neutrons for the RHMMS. Office of Scientific and Technical Information (OSTI), août 1991. http://dx.doi.org/10.2172/6215819.

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