Bibliografías temáticas / Neutrino rates

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Literatura académica sobre el tema "Neutrino rates"

Autor: Grafiati
Publicado: 25 de enero de 2025
Última modificación: 31 de julio de 2025

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Artículos de revistas sobre el tema "Neutrino rates"

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 (1991): 1309–16. http://dx.doi.org/10.1139/p91-196.

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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
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2

Saez, M. M., O. Civitarese, and M. E. Mosquera. "Neutrino mixing in nuclear rapid neutron-capture processes." International Journal of Modern Physics E 29, no. 04 (2020): 2050022. http://dx.doi.org/10.1142/s0218301320500226.

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A possible mechanism for the formation of heavy-mass elements in supernovae is the rapid neutron-capture-mechanism ([Formula: see text]-process). It depends upon the electron-fraction [Formula: see text], a quantity which is determined by beta-decay-rates. In this paper, we focus on the calculation of electroweak decay-rates in presence of massive neutrinos. The resulting expressions are then used to calculate nuclear reactions entering the rapid-neutron capture. We fix the astrophysical parameters to the case of a core-collapse supernova. The neutrino sector includes a mass scheme and mixing
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Chen, Bing-Guang, Tong Liu, Yan-Qing Qi, et al. "Effects of Vertical Advection on Multimessenger Signatures of Black Hole Neutrino-dominated Accretion Flows in Compact Binary Coalescences." Astrophysical Journal 941, no. 2 (2022): 156. http://dx.doi.org/10.3847/1538-4357/aca406.

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Abstract In the coalescence events of binary neutron star (NS) or a black hole (BH) and an NS, a BH hyperaccretion disk might be eventually formed. At very high mass accretion rates, MeV neutrinos will be emitted from this disk, which is called a neutrino-dominated accretion flow (NDAF). Neutrino annihilation in the space out of the disk is energetic enough to launch ultrarelativistic jets to power gamma-ray bursts. Moreover, vertical advection might exist in NDAFs, which can generate the magnetic buoyancy bubbles to release gamma-ray photons. In this paper, we visit the effects of the vertica
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Martínez-Miravé, Pablo, Irene Tamborra, and Alejandro Vigna-Gómez. "Identifying Thorne–Żytkow Objects through Neutrinos." Astrophysical Journal Letters 984, no. 1 (2025): L2. https://doi.org/10.3847/2041-8213/adc8ab.

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Abstract Thorne–Żytkow objects (T Z ̇ Os) have been predicted to form when a neutron star is engulfed by a diffuse, convective giant envelope. Accretion onto a neutron star at a rate that is larger than 10−4 M ⊙ yr−1 is expected to lead to significant emission of neutrinos of all flavors with energy of 1–100 MeV. Since the neutrino signal is expected to largely vary in time (from milliseconds to thousands of years), we outline detection strategies tailored to the signal duration. We find that neutrino detection from T Z ̇ Os up to the Small Magellanic Cloud is within the reach of current- and
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Papoulias, D. K., and T. S. Kosmas. "Nuclear study of the exotic neutrino interactions." HNPS Proceedings 22 (March 8, 2019): 79. http://dx.doi.org/10.12681/hnps.1934.

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Open neutrino physics issues require precision studies, both theoretical and experimental ones, and towards this aim coherent neutral current neutrino-nucleus scattering events are expected to be observed soon. In this work, we explore ν -nucleus processes from a nuclear theory point of view and obtain results with high confidence level based on accurate nuclear structure cross sections calculations. The present study explores the differential event rates as well as the total number of events expected to be measured by nuclear detectors, indicating measurable rates. We concentrate on the possi
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Aiello, S., A. Albert, S. Alves Garre, et al. "Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT." Journal of Cosmology and Astroparticle Physics 2024, no. 04 (2024): 026. http://dx.doi.org/10.1088/1475-7516/2024/04/026.

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Abstract The KM3NeT neutrino telescope is currently being deployed at two different sites in the Mediterranean Sea. First searches for astrophysical neutrinos have been performed using data taken with the partial detector configuration already in operation. The paper presents the results of two independent searches for neutrinos from compact binary mergers detected during the third observing run of the LIGO and Virgo gravitational wave interferometers. The first search looks for a global increase in the detector counting rates that could be associated with inverse beta decay events generated b
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7

Walg, Jonathan, Jon Feldman, and Itzhak Orion. "Decay rate changes in radioactive gamma emission as affected by 18 MeV proton cyclotron." Nuclear Technology and Radiation Protection 39, no. 1 (2024): 1–11. http://dx.doi.org/10.2298/ntrp2401001w.

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Previous efforts to investigate changes in the decay constants of radioactive nuclides discovered that solar flares can temporarily alter radioactive decay rates. Thus, discerning whether external factors affect radioactive decay rates is vital for understanding nuclear processes. This study sought to explore the effect of neutrinos on radioactive nuclei by constructing a gamma radiation detection system that employs a radioactive source in front of a neutrino emission system. Responding to cyclotron operations, each of the four detection systems registered gamma count rate decreases. The resu
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DUTTA, SHARADA IYER, MARY HALL RENO, and INA SARCEVIC. "ULTRAHIGH ENERGY NEUTRINOS." International Journal of Modern Physics A 18, no. 22 (2003): 4085–96. http://dx.doi.org/10.1142/s0217751x03017385.

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The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 1012 GeV, Tests of neutrino oscillations (νμ ↔ ντ) from extragalactic sources of neutrinos are possible with large underground detectors. Measurements of horizontal air shower event rates at neutrino energies above 1010 GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.
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LIU, JING-JING, ZHI-QUAN LUO, HONG-LIN LIU, and XIANG-JUN LAI. "NEUTRINO ENERGY LOSS ON IRON GROUP NUCLEI BY ELECTRON CAPTURE IN STRONG MAGNETIC FIELD AT THE CRUSTS OF NEUTRON STARS." International Journal of Modern Physics A 22, no. 19 (2007): 3305–15. http://dx.doi.org/10.1142/s0217751x07037287.

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The neutrino energy loss rates on iron group nuclei by electron capture are calculated in a strong magnetic field at the crusts of Neutron stars. The results show that the magnetic field has only a slight effect on the neutrino energy loss rates in a range of 108–1013 G on surfaces of the most neutron stars. Whereas for some magnetars which range of the magnetic field is 1013–1018 G, the neutrino energy loss rates of the most iron group nuclei would be debased greatly and may be even decreased for 4 orders of magnitude by the strong magnetic field.
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10

Biondini, S., D. Bödeker, N. Brambilla, et al. "Status of rates and rate equations for thermal leptogenesis." International Journal of Modern Physics A 33, no. 05n06 (2018): 1842004. http://dx.doi.org/10.1142/s0217751x18420046.

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In many realizations of leptogenesis, heavy right-handed neutrinos play the main role in the generation of an imbalance between matter and antimatter in the early Universe. Hence, it is relevant to address quantitatively their dynamics in a hot and dense environment by taking into account the various thermal aspects of the problem at hand. The strong washout regime offers an interesting framework to carry out calculations systematically and reduce theoretical uncertainties. Indeed, any matter–antimatter asymmetry generated when the temperature of the hot plasma [Formula: see text] exceeds the
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Tesis sobre el tema "Neutrino rates"

1

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.

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Thesis (Ph.D.)--Tufts University, 2001.<br>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;
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2

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.

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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
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3

Duan, Mingya. "Study of neutron-star and supernova matter with Skyrme functionals : response functions and new parametrizations." Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPASP171.

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Les étoiles à neutrons sont des objets denses qui sont produits dans des explosions de supernova à effondrement de coeur. Pour la modélisation de la supernova et du refroidissement de l'étoile à neutrons, les taux d'absorption, d'émission et de diffusion des neutrinos jouent un rôle crucial. Dans une grande partie de ces systèmes astrophysiques, les noyaux sont complètement dissous. Dans ce cas, les taux de neutrinos peuvent être directement liés aux fonctions de réponse de la matière nucléaire, calculées aux densités, asymétries et températures correspondantes. Cette thèse développe d'abord l
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4

Houdy, Thibaut. "Testing non-standard neutrino interactions from 8B solar neutrino rate measurement with Borexino to characterization of the 144Ce source of the SOX experiment." Thesis, Sorbonne Paris Cité, 2017. http://www.theses.fr/2017USPCC209/document.

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Le détecteur Borexino, situé au laboratoire souterrain du Gran Sasso (LNGS), mesure les neutrinos solaires depuis 10 ans. Parmi les neutrinos solaires, le spectre continu du 8B jusqu’à 17 MeV permet de tester la zone de transition de l’effet de résonance dans la matière dit effet MSW. Cette nouvelle analyse augmente d’un ordre de grandeur la statistique par rapport à la précédente mesure de Borexino publiée en 2011. Pour ce faire, l’ensemble du volume scintillant a été inclus dans l’analyse, aucune coupure géométrique n’ayant été effectué au dessus de 5 MeV. Cela a permis l’identification d’un
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Heeger, Karsten Miklas. "Model-independent measurement of the neutral-current interaction rate of solar ⁸B neutrinos with deuterium in the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2002. http://hdl.handle.net/1773/9774.

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Sutter, Timothy Charles 1948. "Subsurface thermal neutron production rates." Thesis, The University of Arizona, 1987. http://hdl.handle.net/10150/276631.

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Ground water in excess of one million years old may now be accurately age dated by using the radionuclide Chlorine 36 (36Cl), which has a half-life of 3.01 x 105 years. To maintain a high degree of accuracy in the resultant age it is necessary to take into account the buildup of 36Cl, which is due to thermal neutron activation of 35Cl to 36Cl. The purpose of this research is to determine the thermal neutron flux in various geochemical subsurface environments by conducting field measurements of thermal neutron production rates at discrete locations. These data are then compared with the theoret
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7

ALBANI, GIORGIA. "High-rate thermal neutron gaseous detector for use at neutron spallation sources." Doctoral thesis, Università degli Studi di Milano-Bicocca, 2017. http://hdl.handle.net/10281/158135.

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Il problema, rilevato a livello globale, circa la progressiva riduzione di disponibilità di 3He, ha indotto la comunità scientifica ad intraprendere un’intensa fase di ricerca e sviluppo con lo scopo di trovare tecniche di rivelazione di neutroni alternative a quelle standard basate su 3He. Queste nuove tecnologie, oltre ad avere un’efficienza comparabile a quella dei tubi a 3He, devono risultare idonee ad effettuare misure in sorgenti ad alto flusso di neutroni come la futura European Spallation Source (ESS). In questa tesi di dottorato si ripercorre lo sviluppo di un rivelatore a gas per
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8

Smith, Mark A. "A detector to measure 9Li production rate in liquid scintillator at the earth’s surface by cosmic ray muons." Diss., Kansas State University, 2009. http://hdl.handle.net/2097/1542.

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Doctor of Philosophy<br>Department of Physics<br>Glenn A. Horton-Smith<br>The next generation of nuclear fission reactor based neutrino experiments seeking to measure the Theta-13 mixing angle rely upon measurements made by detectors placed close to the reactor, and therefore less shielded from cosmic ray muons by the earth. 9Li production in liquid scintillator by these cosmic ray muons becomes a serious problem for these experiments that must be dealt with since the 9Li production rate is still a significant fraction of the neutrino interaction rate. This 9Li background reduces the experime
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9

Tyrman, Muriel. "Vers une alternative aux aimants à base de terres rares : hexaferrites nanostructurés et alliages Mn-Al." Thesis, Université Paris-Saclay (ComUE), 2017. http://www.theses.fr/2017SACLV022.

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Dans le cadre d'un projet de transport automobile propre pour la mise en place de véhicules électriques décarbonés grand public, les aimants représentent un enjeu important au niveau des moteurs électriques. Il est alors nécessaire de se passer des aimants à base de terres rares, peu écologiques et dont un seul pays détient le monopole. Deux voies sont explorées ici : la nanostructuration des hexaferrites de type M par frittage flash de type SPS (Spark Plasma Sintering), et la synthèse d'alliages Mn-Al-C par la méthode de la trempe rapide sur roue. Concernant le premier matériau, l'optimisatio
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Harper, Sterling (Sterling M. ). "Calculating reaction rate derivatives in Monte Carlo neutron transport/." Thesis, Massachusetts Institute of Technology, 2016. http://hdl.handle.net/1721.1/106690.

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Thesis: S.M. and S.B., Massachusetts Institute of Technology, Department of Nuclear Science and Engineering, 2016.<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>Cataloged from student-submitted PDF version of thesis.<br>Includes bibliographical references (pages 63-64).<br>An operating nuclear power reactor is a complex system that is sensitive to many material parameters including densities, temperatures, and compositions. There is great interest in solving the neutron transport with Mon
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Libros sobre el tema "Neutrino rates"

1

Davini, Stefano. Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-01213-1.

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Laboratory, Fermi National Accelerator, and United States. National Aeronautics and Space Administration., eds. Cross sections, relic abundance, and detection rates for neutralino dark matter. Fermi National Accelerator Laboratory, 1988.

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Shakshak, Bashir Ibrahim Omar. The measurements of neutron and gamma dose rates in mixed radiation fields, using a liquid scintillation counter. Aston University. Department of Electrical and Electronic Engineering and Applied Physics, 1989.

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J, Decker Arthur, Blue James W, United States. National Aeronautics and Space Administration., and Lewis Research Center, eds. Results of an attempt to measure increased rates of the reaction ²D+²D[reaction direction symbol]³He+n in a nonelectrochemical cold fusion experiment. National Aeronautics and Space Administration, 1989.

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National Aeronautics and Space Administration (NASA) Staff. Cross Sections, Relic Abundance, and Detection Rates for Neutralino Dark Matter. Independently Published, 2018.

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Ellam, Rob. 1. Identical outsides … different insides. Oxford University Press, 2016. http://dx.doi.org/10.1093/actrade/9780198723622.003.0001.

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‘Identical outsides … different insides’ describes the isotopes of hydrogen (protium, deuterium, tritium) and carbon (carbon-12, carbon-13, carbon-14). The isotopes exist due to an extra particle (neutron) or two in the element’s nucleus, which adds extra mass to the atom. Tritium and carbon-14 are both unstable and undergo radioactive decay. There are four types of radioactive decay: α, β, γ (alpha, beta, gamma), and spontaneous fission. Radioactive decay is the process whereby the nucleus of an unstable atom loses energy by emission of ionizing radiation. The rate of the radioactive decay is
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Capítulos de libros sobre el tema "Neutrino rates"

1

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. Springer US, 1996. http://dx.doi.org/10.1007/978-1-4899-1564-1_15.

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Ochoa Ricoux, Juan Pedro. "Predicting the Far Detector Rates." In A Search for Muon Neutrino to Electron Neutrino Oscillations in the MINOS Experiment. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-7949-0_7.

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Davini, Stefano. "Solar Neutrino Observations." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_2.

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Burrows, Adam, and Todd A. Thompson. "Neutrino-Matter Interaction Rates in Supernovae." In Astrophysics and Space Science Library. Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-0-306-48599-2_5.

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Davini, Stefano. "Review of Neutrino Oscillations." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_1.

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Kassim, Hasan Abu, Norhasliza Yusof, R. Hirschi, and P. Eggenberger. "Effects of new nuclear reaction rates on the solar neutrino fluxes." In Synergies between Solar and Stellar Modelling. Springer Netherlands, 2010. http://dx.doi.org/10.1007/978-90-481-9198-7_27.

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Davini, Stefano. "Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_5.

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Klapdor, H. V., K. Grotz, and J. Metzinger. "Microscopic Calculation of Neutrino Capture Rates in 69,71Ga and the Detection of Solar and Galactic Neutrinos." In Weak and Electromagnetic Interactions in Nuclei. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_141.

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Davini, Stefano. "The Borexino Experiment." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_3.

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Davini, Stefano. "The Borexino Detector Response and Simulation." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_4.

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Actas de conferencias sobre el tema "Neutrino rates"

1

Chandler, G. T., K. A. Dunn, M. R. Louthan, et al. "Corrosion Testing in Support of the Accelerator Production of Tritium Program." In CORROSION 2001. NACE International, 2001. https://doi.org/10.5006/c2001-01144.

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Abstract The Accelerator Production of Tritium Project is part of the United States Department of Energy strategy to meet the nation’s tritium needs. The project involves the design of a proton beam accelerator, which will produce tritium through neutron/proton interaction with helium-3. Design, construction and operation of this one-of-a-kind facility will involve the utilization of a wide variety of materials exposed to unique conditions, including elevated temperature and high-energy mixed-proton and -neutron spectra. A comprehensive materials test program was established by the APT project
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Flitton, M. Kay Adler, and Timothy S. Yoder. "Twelve Year Study of Underground Corrosion of Activated Metals." In CORROSION 2012. NACE International, 2012. https://doi.org/10.5006/c2012-01065.

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Abstract The subsurface radioactive disposal facility located at the U.S. Department of Energy’s Idaho site contains neutron-activated metals from non-fuel nuclear-reactor-core components. A long-term corrosion study is being conducted to obtain site-specific corrosion rates to support efforts to more accurately estimate the transfer of activated elements in an arid vadose zone environment. The study uses non-radioactive metal coupons representing the prominent neutron-activated material buried at the disposal location, namely, two types of stainless steels, welded stainless steel, welded nick
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Adler Flitton, M. K., R. E. Mizia, and C. W. Bishop. "Underground Corrosion of Activated Metals in an Arid Vadose Zone Environment." In CORROSION 2002. NACE International, 2002. https://doi.org/10.5006/c2002-02531.

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Abstract The subsurface radioactive disposal site located at the Idaho National Engineering and Environmental Laboratory contains neutron-activated metals from nonfuel nuclear-reactor-core components. A long-term corrosion test is being conducted to obtain site-specific corrosion rates to support efforts to more accurately estimate the transfer of activated elements in an arid vadose zone environment. The tests use nonradioactive metal coupons representing the prominent neutron-activated material buried at the disposal location, namely, Type 304L stainless steel, Type 316L stainless steel, nic
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Haider, H., I. Ruiz Simo, M. Sajjad Athar, et al. "Lepton event rates in neutrino-nucleus DIS." In 12TH INTERNATIONAL WORKSHOP ON NEUTRINO FACTORIES, SUPERBEAMS, AND BETABEAMS: NuFact10. AIP, 2011. http://dx.doi.org/10.1063/1.3644330.

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Karathanou, G. I., V. Tsikoudi, Th Liolios, T. S. Kosmas, Livius Trache, and Sabin Stoica. "Thermonuclear Reaction Rates for Solar Neutrino Processes." In EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (II): Proceedings of the Carpathian Summer School of Physics 2007. AIP, 2008. http://dx.doi.org/10.1063/1.2870466.

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Leung, Chun Sing Jason, and Guey-Lin Lin. "Testing the MSW effect in Supernova Explosion with Neutrino event rates." In 40th International Conference on High Energy physics. Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.390.0145.

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Leung, Chun Sing Jason, KWANG-CHANG LAI, and Guey-Lin Lin. "Testing The MSW Effect in Supernova Explosion with Neutrino Event Rates." In European Physical Society Conference on High Energy Physics. Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.364.0417.

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Nabi, Jameel-Un, Hajime Susa, Marcel Arnould, et al. "Neutrino Energy Loss Rates due to [sup 54,55,56]Fe in Stellar Environment." In TOURS SYMPOSIUM ON NUCLEAR PHYSICS AND ASTROPHYSICS—VII. AIP, 2010. http://dx.doi.org/10.1063/1.3455932.

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Paar, N., D. Vretenar, T. Marketin, et al. "Neutrino-nucleus reaction rates based on the relativistic quasiparticle random phase approximation." In FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP, 2008. http://dx.doi.org/10.1063/1.2939358.

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Marketin, Tomislav, Lutz Huther, Jelena Petković, Nils Paar, and Gabriel Martínez-Pinedo. "Beta decay rates of neutron-rich nuclei." In CETUP* 2015 – WORKSHOP ON DARK MATTER, NEUTRINO PHYSICS AND ASTROPHYSICS AND PPC 2015 – IXTH INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY. Author(s), 2016. http://dx.doi.org/10.1063/1.4953298.

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Informes sobre el tema "Neutrino rates"

1

Iverson, Erik B. Order-of-Magnitude Estimate of Fast Neutron Recoil Rates in Proposed Neutrino Detector at SNS. Office of Scientific and Technical Information (OSTI), 2006. http://dx.doi.org/10.2172/974593.

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Goldman, Jesse Matthew. A Next-to-leading order QCD analysis of charged current event rates from neutrino N deep inelastic scattering at the Fermilab Tevatron. Office of Scientific and Technical Information (OSTI), 2000. http://dx.doi.org/10.2172/1421436.

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Shores, Erik Frederick. Tabulated Neutron Emission Rates for Plutonium Oxide. Office of Scientific and Technical Information (OSTI), 2017. http://dx.doi.org/10.2172/1372807.

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Favorite, Jeffrey A. SENSMG: First-Order Sensitivities of Neutron Reaction Rates, Reaction-Rate Ratios, Leakage, keff, and α Using PARTISN. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1333129.

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Favorite, Jeffrey A. (U) SENSMG: First-Order Sensitivities of Neutron Reaction Rates, Reaction-Rate Ratios, Leakage, keff, α, and Subcritical Multiplication Using PARTISN. Office of Scientific and Technical Information (OSTI), 2019. http://dx.doi.org/10.2172/1530773.

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Favorite, Jeffrey. (U) SENSMG: First-Order Sensitivities of Neutron Reaction Rates, Reaction-Rate Ratios, Leakage, keff, α, and Subcritical Multiplication Using PARTISN. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1884735.

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Smith, Donald L. Observations on the Effects of 252Cf Spontaneous-Fission Neutron Spectrum Uncertainties on Uncertainties in Calculated Spectrum-Average Cross Sections for Reactions in the Neutron Dosimetry Library IRDFF-II. IAEA Nuclear Data Section, 2022. http://dx.doi.org/10.61092/iaea.wx80-dm11.

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Resumen
The Neutron Dosimetry Library IRDFF-II was released in January 2020, and was subsequently documented by an article published in the Nuclear Data Sheets by A. Trkov et al. The development of this library, under the auspices of the IAEA Nuclear Data Section, entailed extensive effort to assemble and examine the available, relevant experimental data, as well as to select and validate the best available cross-section evaluations, for some 110 neutron reaction processes included in this library. Part of the validation process for this library entailed comparing experimental and evaluated differenti
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Holman-Abbott, Michelle, and Alan Boone. Portable Neutron Dose Rate Instrument Evaluation. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1462170.

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Couture, Aaron Joseph. A Simple Correlation for Neutron Capture Rates from Nuclear Masses. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1418787.

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Long, Grace, and Alexis Trahan. Parameter Affecting Neutron Coincidence Rates Detected from Spent Nuclear Fuel. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1645058.

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