Relevant bibliographies by topics / Neutrino interactions

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Neutrino interactions'

Author: Grafiati
Published: 4 June 2021
Last updated: 29 July 2024

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Neutrino interactions.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Neutrino interactions"

1

Hargrove, C. K., and D. J. Paterson. "Solar-neutrino neutral-current detection methods in the Sudbury neutrino observatory." Canadian Journal of Physics 69, no. 11 (November 1, 1991): 1309–16. http://dx.doi.org/10.1139/p91-196.

Full text
Abstract:
The Sudbury Neutrino Observatory will study the solar-neutrino problem through the detection of charged-current (CC), neutral-current (NC), and elastic-scattering (ES) interactions of solar neutrinos with heavy water. The measurement of the NC rate relative to the CC rate provides a nearly model-independent method of observing neutrino oscillations. The NC interaction breaks up the deuteron producing a neutron and a proton. The interaction rate in the original design is measured by observing Čerenkov light from showers produced by neutron-capture γ rays from the capture of the NC neutrons by a selected additive to the heavy water. These signals overlap the CC and ES signals, so that the measurement of the NC rate requires the subtraction of two signals obtained at different times. This paper describes our investigation of an alternate detection method in which the thermalized neutrons are captured by (n, α) or (n, p) reactions on light nuclei. The resulting charged-particle products are uniquely detected by scintillators or proportional counters, completely separating this NC signal from the CC and ES Čerenkov signals, thus simplifying its measurement, improving its significance, and allowing observation of otherwise unobservable short-term NC fluctuations. Although background rates for the new techniques have not yet been determined, the experimental advantages justify further development work.
APA, Harvard, Vancouver, ISO, and other styles
2

Caravaca, J. "SNO: Recent new results." International Journal of Modern Physics A 35, no. 34n35 (December 15, 2020): 2044012. http://dx.doi.org/10.1142/s0217751x20440121.

Full text
Abstract:
The Sudbury Neutrino Observatory (SNO), whose main purpose was to study the neutrinos produced in the Sun, demonstrated that neutrinos can change flavor and, thus, they are massive particles. SNO detected and recorded neutrino and cosmic ray interactions from 1999 to 2006 and several analyses have been completed in the past year using legacy data. We present the results of the most recent ones: the measurements of neutron production in atmospheric neutrino interactions and neutron production by cosmic muons, a search for Lorentz symmetry violation in neutrino oscillations and a search for neutrino decay. A few other analyses are ongoing and we comment about their goal and status.
APA, Harvard, Vancouver, ISO, and other styles
3

Abe, Seisho. "Nuclear de-excitation associated with neutrino-carbon interactions." Journal of Physics: Conference Series 2156, no. 1 (December 1, 2021): 012189. http://dx.doi.org/10.1088/1742-6596/2156/1/012189.

Full text
Abstract:
Abstract Neutrino interactions in low energy regions below 30 MeV, where the experimental searches for supernova relic neutrino are conducted, have a large uncertainty due to complicated nuclear effects such as the Pauli blocking effect and de-excitation of a residual nucleus. Understanding the effect of nuclear de-excitation is especially critical since neutrons measured by liquid scintillator detectors can be emitted via de-excitation. We build a systematic method to predict nuclear de-excitation associated with neutrino-carbon interaction using TALYS and Geant4. This prediction is combined with the results of neutrino event generators, and we find a large increase in neutron multiplicity.
APA, Harvard, Vancouver, ISO, and other styles
4

Balantekin, A. Baha, Michael J. Cervia, Amol V. Patwardhan, Rebecca Surman, and Xilu Wang 王夕露. "Collective Neutrino Oscillations and Heavy-element Nucleosynthesis in Supernovae: Exploring Potential Effects of Many-body Neutrino Correlations." Astrophysical Journal 967, no. 2 (May 28, 2024): 146. http://dx.doi.org/10.3847/1538-4357/ad393d.

Full text
Abstract:
Abstract In high-energy astrophysical processes involving compact objects, such as core-collapse supernovae or binary neutron star mergers, neutrinos play an important role in the synthesis of nuclides. Neutrinos in these environments can experience collective flavor oscillations driven by neutrino–neutrino interactions, including coherent forward scattering and incoherent (collisional) effects. Recently, there has been interest in exploring potential novel behaviors in collective oscillations of neutrinos by going beyond the one-particle effective or “mean-field” treatments. Here, we seek to explore implications of collective neutrino oscillations, in the mean-field treatment and beyond, for the nucleosynthesis yields in supernova environments with different astrophysical conditions and neutrino inputs. We find that collective oscillations can impact the operation of the ν p-process and r-process nucleosynthesis in supernovae. The potential impact is particularly strong in high-entropy, proton-rich conditions, where we find that neutrino interactions can nudge an initial ν p-process neutron-rich, resulting in a unique combination of proton-rich low-mass nuclei as well as neutron-rich high-mass nuclei. We describe this neutrino-induced neutron-capture process as the “ν i-process.” In addition, nontrivial quantum correlations among neutrinos, if present significantly, could lead to different nuclide yields compared to the corresponding mean-field oscillation treatments, by virtue of modifying the evolution of the relevant one-body neutrino observables.
APA, Harvard, Vancouver, ISO, and other styles
5

Nakarmi, Prabandha, and Jeevan Jyoti Nakarmi. "Significance of neutrino-neutrino interaction in neutrino oscillation in core-collapse supernova." BIBECHANA 12 (December 17, 2014): 89–95. http://dx.doi.org/10.3126/bibechana.v12i0.11780.

Full text
Abstract:
We study the possibility of neutrino-neutrino interaction inside the neutrino core of supernova (ρ ≥ 1010 g/cc) and outside the neutrinosphere. The angular dependence of the neutrino-neutrino interaction Hamiltonian causes multi-angle effects that can lead either to oscillation or free streaming of neutrinos. If the angle between interactions is π/2, the neutrinos are trapped inside neutrino core and chances of oscillation increases due to interaction. As the angle gradually changes, the chance of oscillation decreases and free streaming of neutrino can be observed out of core of supernova as shock waves.DOI: http://dx.doi.org/10.3126/bibechana.v12i0.11780 BIBECHANA 12 (2015) 89-95
APA, Harvard, Vancouver, ISO, and other styles
6

Esteban, Ivan, Sujata Pandey, Vedran Brdar, and John F. Beacom. "Astrophysical neutrino self-interactions in the high-statistics era." Journal of Physics: Conference Series 2156, no. 1 (December 1, 2021): 012103. http://dx.doi.org/10.1088/1742-6596/2156/1/012103.

Full text
Abstract:
Abstract Do neutrinos have sizable self-interactions? They might. Laboratory constraints are weak, so strong effects are possible in astrophysical environments and the early universe. Observations with neutrino telescopes can provide an independent probe of neutrino self (“secret”) interactions, as the sources are distant and the cosmic neutrino background intervenes. We define a roadmap for making decisive progress on testing these interactions. This progress will be enabled by IceCube-Gen2 observations of high-energy astrophysical neutrinos. Critical to this is our comprehensive treatment of the theory, taking into account previously neglected or overly approximated effects, as well as including realistic detection physics. We show that IceCube-Gen2 can realize the full potential of neutrino astronomy for testing neutrino self-interactions, being sensitive to cosmologically relevant interaction models.
APA, Harvard, Vancouver, ISO, and other styles
7

An, Rui, Vera Gluscevic, Ethan O. Nadler, and Yue Zhang. "Can Neutrino Self-interactions Save Sterile Neutrino Dark Matter?" Astrophysical Journal Letters 954, no. 1 (August 31, 2023): L18. http://dx.doi.org/10.3847/2041-8213/acf049.

Full text
Abstract:
Abstract Sterile neutrinos only interact with the standard model through the neutrino sector, and thus represent a simple dark matter (DM) candidate with many potential astrophysical and cosmological signatures. Recently, sterile neutrinos produced through self-interactions of active neutrinos have received attention as a particle candidate that can yield the entire observed DM relic abundance without violating the most stringent constraints from X-ray observations. We examine consistency of this production mechanism with the abundance of small-scale structure in the universe, as captured by the population of ultrafaint dwarf galaxies orbiting the Milky Way, and derive a lower bound on the sterile-neutrino particle mass of 37 keV. Combining these results with previous collider and X-ray limits excludes 100% sterile-neutrino DM produced by strong neutrino self-coupling, mediated by a heavy (≳1 GeV) scalar; however, data permits sterile-neutrino DM production via a light mediator.
APA, Harvard, Vancouver, ISO, and other styles
8

Carpio, Jose Alonso, and Kohta Murase. "Simulating neutrino echoes induced by secret neutrino interactions." Journal of Cosmology and Astroparticle Physics 2023, no. 02 (February 1, 2023): 042. http://dx.doi.org/10.1088/1475-7516/2023/02/042.

Full text
Abstract:
Abstract New neutrino interactions beyond the Standard Model (BSM) have been of much interest in not only particle physics but also cosmology and astroparticle physics. We numerically investigate the time delay distribution of astrophysical neutrinos that interact with the cosmic neutrino background. Using the Monte Carlo method, we develop a framework that enables us to simulate the time-dependent energy spectra of high-energy neutrinos that experience even multiple scatterings en route and to handle the sharp increase in the cross section at the resonance energy. As an example, we focus on the case of secret neutrino interactions with a scalar mediator. While we find the excellent agreement between analytical and simulation results for small optical depths, our simulations enable us to study optically thick cases that are not described by the simplest analytic estimates. Our simulations are used to understand effects of cosmological redshifts, neutrino spectra and flavors. The developments will be useful for probing BSM neutrino interactions with not only current neutrino detectors such as IceCube and Super-Kamiokande but also future neutrino detectors such as IceCube-Gen2 and Hyper-Kamiokande.
APA, Harvard, Vancouver, ISO, and other styles
9

Mazumdar, Arindam, Subhendra Mohanty, and Priyank Parashari. "Flavour specific neutrino self-interaction: H 0 tension and IceCube." Journal of Cosmology and Astroparticle Physics 2022, no. 10 (October 1, 2022): 011. http://dx.doi.org/10.1088/1475-7516/2022/10/011.

Full text
Abstract:
Abstract Self-interaction in the active neutrinos is studied in the literature to alleviate the H_0 tension. Similar self-interaction can also explain the observed dips in the flux of the neutrinos coming from the distant astro-physical sources in IceCube detectors. In contrast to the flavour universal neutrino interaction considered for solving the H 0 tension, which is ruled out from particle physics experiments, we consider flavour specific neutrino interactions. We show that the values of self-interaction coupling constant and mediator mass required for explaining the IceCube dips are inconsistent with the strong neutrino self-interactions preferred by the combination of BAO, HST and Planck data. However, the required amount of self-interaction between tau neutrinos (ντ ) in inverted hierarchy for explaining IceCube dips is consistent with the moderate self-interaction region of cosmological bounds at 1-σ level. For the case of other interactions and hierarchies, the IceCube preferred amount of self-interaction is consistent with moderate self-interaction region of cosmological bounds at 2-σ level only.
APA, Harvard, Vancouver, ISO, and other styles
10

Kolbe, E., and T. S. Kosmas. "Recent highlights on neutrino-nucleus interactions." HNPS Proceedings 9 (February 11, 2020): 63. http://dx.doi.org/10.12681/hnps.2776.

Full text
Abstract:
The recent developments on neutrino-nucleus interactions at low and intermediate energies are reviewed and discussed in conjunction with the recent data of atmospheric, solar, and accelerator neutrino experiments. The theoretical nuclear physics approaches used to interpret and predict phenomena for which neutrinos play a crucial role are also investigated. We emphasize on the implications of neutrino reactions and properties into the astrophysical phenomena and atmospheric neutrino problems.
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Neutrino interactions"

1

Szafron, Robert. "General description of neutrino oscillations with non-standard interactions." Doctoral thesis, Katowice : Uniwersytet Śląski, 2012. http://hdl.handle.net/20.500.12128/5275.

Full text
Abstract:
We present a formalism describing neutrino oscillations in any application beyond the Standard Model theory. Instead of using the standard pure states approach, we apply the density matrix formalism. In general, in New Physics models, neutrino states are no longer as pure as they are in the Standard Model. We discuss the details of the appearance of a mixed state, following which possible New Physics effects are taken at the levels of both the production and detection processes. We present a number of examples of calculations with our formalism, using muons as a source of neutrinos and different detection process. We also show the connection between normal formulae, derived by assuming pure states, and proper results based on the density matrix approach. The difference occurs at the second order in parameters describing the departure from the Standard Model. Finally, as an application of our formalism, we also demonstrate that it is possible to distinguish Dirac and Majorana neutrinos in oscillations when New Physics scalar interactions are present.
APA, Harvard, Vancouver, ISO, and other styles
2

Tsang, Ka-vang, and 曾嘉宏. "A search for periodic neutrino signals and gamma-ray burst neutrinos with the Sudbury Neutrino Observatory." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2005. http://hub.hku.hk/bib/B3194324X.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Tsang, Ka-vang. "A search for periodic neutrino signals and gamma-ray burst neutrinos with the Sudbury Neutrino Observatory." Click to view the E-thesis via HKUTO, 2005. http://sunzi.lib.hku.hk/hkuto/record/B3194324X.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Roda, Marco. "Study of multiple vertices neutrino interactions in the OPERA experiment." Doctoral thesis, Università degli studi di Padova, 2016. http://hdl.handle.net/11577/3426767.

Full text
Abstract:
OPERA is a long baseline neutrino experiment designed for tau neutrino searches in an almost pure muon neutrino beam. The detection is performed on an event-by-event basis which is possible thanks to the high spatial resolution of the detector. In fact, the set-up is able to observe very short decaying particles produced in neutrino interactions, such as tau or charmed particles. In particular, the experiment searches for events with one secondary vertex within 1 mm from the primary one. An event was recorded with an unexpected topology: instead of one secondary vertex it has two. Such an event was completely unexpected and a totally new analysis was required in order to understand its nature. The possibilities taken into account include most of the combinations of tau, charmed particle and hadron re-interaction within the lead. The new software, based on GEANT4, was set-up and successfully tested using a dedicated OPERA test beam. Thus, an ad hoc Monte Carlo generation was prepared in order to describe the properties of such a rare observation. Finally, a sample having the interesting topology was obtained and a blind procedure for the event identification could be developed. The event turned out to be very likely an tau neutrino interaction with charm production with a significance close to 3.5 sigma.
OPERA è un esperimento per lo studio di neutrini da fascio progettato per ricerca di neutrini del tau in un fascio quasi puro di neutrini muonici. La ricerca è basata su un’analisi evento per evento che è resa possibile dall’elevata risoluzione spaziale del rivelatore. Infatti, l’apparato è in grado di osservare particelle emesse durante un’interazione di neutrino che decadono entro brevi distanze. In particolare, l’esperimento ricerca eventi che presentano vertici secondari entro circa un millimetro dal vertice primario di interazione. Un evento interessante è stato osservato con una topologia inaspettata: invece un solo vertice secondario ne sono stati osservati due. Questo tipo di eventi era completamente inaspettato e una nuova analisi era necessaria per capire la natura dell’evento. Le possibilità considerate includono quasi tutte le combinazioni di tau, particelle charmate e reinterazioni adroniche nel piombo. Un nuovo algoritmo di simulazione, basato su GEANT4, è stato sviluppato e testato con successo usando i dati di uno dei test beam di OPERA. Quindi, una nuova produzione Monte Carlo è stata preparata per poter descrivere le proprietà di questo raro fenomeno. Infine, è stata preparata un’analisi per l’identificazione dell’evento osservato. L’evento è risultato essere molto probabilmente un’interazione di neutrino del tau con produzione di charm, con una significanza di quasi 3.5 sigma.
APA, Harvard, Vancouver, ISO, and other styles
5

George, Jeffrey S. "Experimental study of the atmospheric [Nu][mu]/[Nu]e ratio in the multi-GeV energy range /." Thesis, Connect to this title online; UW restricted, 1998. http://hdl.handle.net/1773/9752.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Ahlgren, Björn. "Astrophysical Constraints on Secret Neutrino Interactions." Thesis, KTH, Teoretisk fysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-137181.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Chung, Jin-Hyuk. "Search for neutron oscillation and study of neutrino reaction rates using multiprong events in Soudan 2 /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2001.

Find full text
Abstract:
Thesis (Ph.D.)--Tufts University, 2001.
Adviser: W. Anthony Mann. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 125-130). Access restricted to members of the Tufts University community. Also available via the World Wide Web;
APA, Harvard, Vancouver, ISO, and other styles
8

Kikawa, Tatsuya. "Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment." 京都大学 (Kyoto University), 2015. http://hdl.handle.net/2433/195958.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Ferchichi, Chiraz. "Study of neutrino interactions in the near detector of T2K." Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112106.

Full text
Abstract:
L’expérience T2K étudie les propriétés des neutrinos, en particulier le phénomène d’oscillation des neutrinos. Se déroulant au Japon, elle utilise un faisceau de neutrinos muoniques produit par le complexe d’accélérateur J-PARC, un détecteur proche, ND280 sur le site même de J-PARC pour caractériser le faisceau, et un détecteur lointain, Super-Kamiokande situé à 295 km pour mesurer les oscillations de neutrinos. Le détecteur proche permet également d’étudier les interactions des neutrinos et cette thèse porte sur la mesure des sections efficaces de diffusion profondément inélastique des neutrinos muoniques.Le manuscrit introduit d’abord la physique des neutrinos, puis l’expérience T2K et en particulier les chambres à projection temporelles du détecteur proche, en insistant sur la vérification de la qualité des données, dont j’avais la charge. L’analyse porte sur les données de T2K enregistrées jusqu’en 2013. La sélection d’interactions de neutrinos muoniques par courant chargé est ensuite présentée, ainsi qu’une étude préliminaire de la sélection d’interactions de neutrinos muoniques par courant chargé avec production d’un pion neutre. Un critère portant sur la multiplicité des traces permet d’enrichir le premier lot en interactions correspondant à une diffusion profondément inélastique de neutrinos. Finalement un ajustement, validé d’abord sur des données simulées, permet d’extraire les sections efficaces de diffusion profondément inélastique des neutrinos muoniques
The T2K experiment studies the properties of neutrinos, particularly neutrino oscillations. It takes place in Japan and uses a muonic neutrino beam produced by the J-PARC accelerator complex, a near detector, ND280 on the J-PARC site in order to characterise the beam, and a far detector, Super-Kamiokande 295 km away in order to measure the neutrino oscillations. The near detector is also used to study the neutrino interactions and the goal of this thesis is the measurement of muonic neutrino deep inelastic scattering cross sections.The thesis first introduces neutrino physics, then the T2K experiment and more particularly the time projection chambers of the near detector, and its data quality checking that I was in charge of. The analysis is based on the T2K data recorded until 2013. The selection of charged current muonic neutrino interactions is then presented, as well as a preliminary study of the selection of charged current muonic neutrino interactions with the production of a neutral pion. A criterion on track multiplicity allows enriching the former sample in interactions corresponding to a neutrino deep inelastic scattering. Finally a fit, first validated on simulated data, allows the extraction of the muonic neutrino deep inelastic scattering cross sections
APA, Harvard, Vancouver, ISO, and other styles
10

Cuha, Volkan. "Study Of Neutrino Interactions In The Chorus Experiment." Master's thesis, METU, 2006. http://etd.lib.metu.edu.tr/upload/12607891/index.pdf.

Full text
Abstract:
The emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS between the years 1994 and 1997. In total about 130.000 neutrino interactions were located in the nuclear emulsion target and fully reconstructed. Detailed DATA and Monte Carlo (MC) comparisons were done in order to test reliability of the detector simulation. There is reasonable agreement between DATA and MC. The ratio of deep inelastic neutral-current (NC) to the deep inelastic (DIS) charged-current(CC) $nu_{mu}$ interactions was measured to be frac{NC_{dis}}{CC_{dis}}=0.350pm0.003$. This measurement was compared with the previous measurements. Based on three double charm decays found in NC interactions we measured the ratio of double charm cross-section in NC $nu_{mu}$ interactions to be [ frac{sigma (cbar{c}nu_mu)}{sigma_{NC}}=(3.37^{+3.06}_{-2.51}(stat.)pm 0.51(syst.))times 10^{-3}. ] One double charm decay has been observed in CC $nu_{mu}$ interactions the upper limit on associated charm production in $nu_{mu}$ CC interaction has been found to be [ frac{sigma cbar{c}mu^{-})}{sigma_{CC}}<
9.69 times 10^{-4}. ] at 90% C.L.
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "Neutrino interactions"

1

1930-, Winter Klaus, ed. Neutrino physics. Cambridge [England]: Cambridge University Press, 1991.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
2

Federico, Sánchez, ed. Sixth International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region: NUINT-09, Sitges (Barcelona), Spain, 18-22 May 2009. Melville, N.Y: American Institute of Physics, 2009.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
3

International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region (3rd 2004 Assergi, Italy). NuInt04: Proceedings of the Third International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region : Assergi, Italy, 17-21 March 2004. [Amsterdam]: Elsevier, 2005.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
4

International Workshop on Neutrino-Nucleus Interactions in the Few GeV Region (2001 Tsukuba, Japan). Neutrino-nucleus interactions in the few GeV region: Proceedings of the First International Workshop on Neutrino-Nucleus Interactions in the Few GeV Region : KEK, Tsukuba, Japan, 13-16 December, 2001. Amsterdam: North-Holland, 2002.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
5

P, Zeller Geralyn, Morfín Jorge G, and Cavanna F, eds. Neutrino-nucleus interactions in the Few-GeV region: Nulnt07, the 5th International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region, Batavia, Illinois, 30 May-3 June 2007. Melville, N.Y: American Institute of Physics, 2007.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
6

International Workshop on Neutrino-Nucleus Interactions in the Few GeV Region (2001 Tsukuba, Japan). Neutrino-nucleus interactions in the few GeV region: Proceedings of the First International Workshop on Neutrino-Nucleus Interactions in the Few GeV Region : KEK, Tsukuba, Japan, 13-16 December, 2001. Amsterdam: North-Holland, 2002.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
7

Mistry, Krishan V. J. Exploring Electron–Neutrino–Argon Interactions. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-19572-3.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Suzuki, Atsuto. Nyūtorino de wakaru uchū, soryūshi no nazo. Tōkyō-to Chiyoda-ku: Shūeisha, 2013.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
9

L, Bergström, ed. Neutrino physics: Proceedings of Nobel Symposium 129 : Haga Slott, Enköping, Sweden, August 19-24, 2004. New Jersey: World Scientific, 2005.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
10

Jayawardhana, Ray. Neutrino hunters: The thrilling chase for a ghostly particle to unlock the secrets of the universe. Toronto: HarperCollins Publishers Ltd., 2013.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
More sources

Book chapters on the topic "Neutrino interactions"

1

Mistry, Krishan V. J. "Neutrino Interactions." In Exploring Electron–Neutrino–Argon Interactions, 15–32. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-19572-3_3.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Baldo-Ceolin, Milla. "Neutrino Masses and Mixing from Neutrino Oscillations." In 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.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Grieder, Peter K. F. "Muon and Neutrino Interactions." In Exentsive Air Showers and High Energy Phenomena, 205–36. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76941-5_5.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Grange, Joseph. "Neutrino Interactions in MiniBooNE." In First Measurement of the Muon Anti-Neutrino Charged Current Quasielastic Double-Differential Cross Section, 29–38. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-09573-8_4.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Suekane, Fumihiko. "Neutrinos and Weak Interactions in the Standard Model." In Neutrino Oscillations, 7–29. Tokyo: Springer Japan, 2015. http://dx.doi.org/10.1007/978-4-431-55462-2_2.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Valle, J. W. F. "Weak Interactions and Solar Neutrinos: Testing the Oscillation Hypothesis." In Neutrino Physics, 258–68. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73679-7_26.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Mistry, Krishan V. J. "Overview of Neutrino Properties." In Exploring Electron–Neutrino–Argon Interactions, 3–13. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-19572-3_2.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Megias, G. D., S. Dolan, and S. Bolognesi. "Modeling Neutrino-Nucleus Interactions for Neutrino Oscillation Experiments." In Springer Proceedings in Physics, 149–51. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-22204-8_12.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Mikheyev, S. P., and A. Yu Smirnov. "Neutrino Oscillations in Matter." In Weak and Electromagnetic Interactions in Nuclei, 710–17. Berlin, Heidelberg: Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_138.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Gandhi, Raj, Chris Quigg, M. H. Reno, and Ina Sarcevic. "Ultrahigh-Energy Neutrino Interactions and Neutrino Telescope Event Rates." In Neutrino Mass, Dark Matter, Gravitational Waves, Monopole Condensation, and Light Cone Quantization, 121–30. Boston, MA: Springer US, 1996. http://dx.doi.org/10.1007/978-1-4899-1564-1_15.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Neutrino interactions"

1

Kopeliovich, B. Z., I. K. Potashnikova, Iván Schmidt, and M. Siddikov. "Diffractive neutrino interactions." In DIFFRACTION 2012: International Workshop on Diffraction in High Energy Physics. AIP, 2013. http://dx.doi.org/10.1063/1.4802117.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Mertens, Susanne, and Stefano Morisi. "Neutrino masses, states and interactions." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0076.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

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

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Forastieri, Francesco. "Planck constraints on secret neutrino interactions." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0084.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

McKellar, Bruce H. J. "Tritium decay, neutrino mixing and neutrino interactions." In The third international symposium on symmetries in subatomic physics. AIP, 2000. http://dx.doi.org/10.1063/1.1330902.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Gariazzo, Stefano, and Monica Sisti. "Neutrino masses, states and interactions: session summary." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0079.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Ghosh, Subhajit, Rishi Khatri, and Tuhin S. Roy. "Dark neutrino interactions make gravitational waves blue." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0086.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Katori, Teppei. "Hadronization processes in neutrino interactions." In 16th International Workshop on Neutrino Factories and Future Neutrino Beam Facilities. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.226.0053.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Rodrigues, P. A. "Measuring neutrino-nucleus interactions with MINERνA." In XXVI INTERNATIONAL CONFERENCE ON NEUTRINO PHYSICS AND ASTROPHYSICS: Neutrino 2014. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4915558.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Mosel, Ulrich, TINA LEITNER, Oliver Buss, and Luis Alvarez-Ruso. "Neutrino interactions with nuclei." In 10th International Workshop on Neutrino Factories, Super beams and Beta beams. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.074.0009.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Reports on the topic "Neutrino interactions"

1

Kamyshkov, Yuri, and Thomas Handler. Neutrino Interactions. Office of Scientific and Technical Information (OSTI), October 2016. http://dx.doi.org/10.2172/1329518.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Dicus, D. A., and W. W. Repko. Photon-neutrino interactions. Office of Scientific and Technical Information (OSTI), December 1997. http://dx.doi.org/10.2172/555478.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Pal, P. B. Neutrino interactions in matter. Office of Scientific and Technical Information (OSTI), March 1993. http://dx.doi.org/10.2172/10161062.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Pal, P. B. Neutrino interactions in matter. Office of Scientific and Technical Information (OSTI), March 1993. http://dx.doi.org/10.2172/7368704.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Abbasabadi, A., A. Devoto, D. A. Dicus, and W. W. Repko. High energy photon-neutrino interactions. Office of Scientific and Technical Information (OSTI), July 1998. http://dx.doi.org/10.2172/639760.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Sharma, Richa. Study of Neutrino Interactions in MINOS. Office of Scientific and Technical Information (OSTI), January 2014. http://dx.doi.org/10.2172/1209536.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Abashian, A. Study of electron and neutrino interactions. Office of Scientific and Technical Information (OSTI), March 1997. http://dx.doi.org/10.2172/461290.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Grossman, yuval. Neutrino propagation in matter with general interactions. Office of Scientific and Technical Information (OSTI), April 1999. http://dx.doi.org/10.2172/10027.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Dishaw, j. The Production of Neutrinos and Neutrino-like Particles in Proton-Nucleus Interactions. Office of Scientific and Technical Information (OSTI), June 2018. http://dx.doi.org/10.2172/1453961.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Oltman, Edward. Nucleon Structure Functions from High-Energy Neutrino and Anti-Neutrino Interactions in Iron. Office of Scientific and Technical Information (OSTI), January 1989. http://dx.doi.org/10.2172/1427781.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Neutrino interactions' for particular source types:
Journal articles Dissertations / Theses Books
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography