Literatura académica sobre el tema "Neutron emissions"
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Artículos de revistas sobre el tema "Neutron emissions"
Petrucci, Andrea, Alberto Rosada y Emilio Santoro. "Asymmetric neutron emissions from sonicated steel". Modern Physics Letters B 29, n.º 14 (29 de mayo de 2015): 1550067. http://dx.doi.org/10.1142/s0217984915500670.
Texto completoAlbertini, G., V. Calbucci y F. Cardone. "Statistics of piezonuclear emissions: early results". Modern Physics Letters B 28, n.º 05 (18 de febrero de 2014): 1450036. http://dx.doi.org/10.1142/s0217984914500365.
Texto completoPetrucci, Andrea y Alberto Rosada. "Ultrasonic Neutron Emissions". Journal of Advanced Physics 5, n.º 1 (1 de marzo de 2016): 63–68. http://dx.doi.org/10.1166/jap.2016.1246.
Texto completoPozzi, Sara A., Brian Wieger, Andreas Enqvist, Shaun D. Clarke, Marek Flaska, Matthew Marcath, Edward Larsen, Robert C. Haight y Enrico Padovani. "Correlated Neutron Emissions from252Cf". Nuclear Science and Engineering 178, n.º 2 (octubre de 2014): 250–60. http://dx.doi.org/10.13182/nse13-96.
Texto completoBradnam, Steven C., Vytautas Astromskas, Zamir Ghani, Mark R. Gilbert, Malcolm J. Joyce y Lee W. Packer. "DEVELOPMENT AND EXPERIMENTAL VALIDATION OF RESPONSE MODELLING FOR TIME-OF-FLIGHT NEUTRON DETECTION AND IMAGING SYSTEMS". EPJ Web of Conferences 247 (2021): 16001. http://dx.doi.org/10.1051/epjconf/202124716001.
Texto completoMuraki, Y., K. Koga, T. Goka, H. Matsumoto, T. Obara, O. Okudaira, S. Shibata y T. Yamamoto. "Measurement by FIB on the ISS: Two Emissions of Solar Neutrons Detected?" Advances in Astronomy 2012 (2012): 1–14. http://dx.doi.org/10.1155/2012/379304.
Texto completoVartanyan, David, Adam Burrows y David Radice. "Temporal and angular variations of 3D core-collapse supernova emissions and their physical correlations". Monthly Notices of the Royal Astronomical Society 489, n.º 2 (21 de agosto de 2019): 2227–46. http://dx.doi.org/10.1093/mnras/stz2307.
Texto completoMohindroo, Kumar S., Yaron Danon, Ezekiel Blain, Matthew Devlin y Keegan J. Kelly. "Quasi-differential neutron induced neutron emissions from 235U, and 239Pu". Annals of Nuclear Energy 165 (enero de 2022): 108647. http://dx.doi.org/10.1016/j.anucene.2021.108647.
Texto completoKromar, Marjan y Bojan Kurinčič. "Assessment of the Photon and Neutron Source Term for the NPP Krško Spent Fuel". Journal of Energy - Energija 68, n.º 2-3 (8 de julio de 2022): 184–98. http://dx.doi.org/10.37798/2019682-3202.
Texto completoKimura, Shigeo S. "High-energy emissions from neutron star mergers". EPJ Web of Conferences 210 (2019): 03001. http://dx.doi.org/10.1051/epjconf/201921003001.
Texto completoTesis sobre el tema "Neutron emissions"
Khrbish, Yabia Saleh. "Application of neutron and proton induced prompt emissions for elemental analysis". Thesis, University of Surrey, 1987. http://epubs.surrey.ac.uk/844238/.
Texto completoSteer, Steven John. "Isomer decay spectroscopy of N<126 neutron-rich nuclei". Thesis, University of Surrey, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.493243.
Texto completoThomson, Brent Wayne. "Determining the origin and possible mechanisms of QPOS in x-ray emissions of neutron stars and black holes". Thesis, The University of North Dakota, 2015. http://pqdtopen.proquest.com/#viewpdf?dispub=3681134.
Texto completoQPOs (Quasi-Periodic Oscillations) are time oscillations that appear in the light curve of observational data in x-ray bands. They are of mysterious origin although they are believed to be a result of the intense gravity around neutron stars and black holes and emit x-rays from accretion disks. I investigate a derived ratio between two periods has been found in the QPO data. The two periods, which appear as peaks in the power density spectrum have been found to be in a 3:2 ratio and can possibly distinguish theoretical models. In the work presented here, two physical approaches are developed that can explain the integer resonance ratio. One is a cusp layer model, which is based on a boundary layer model that uses the physical conditions at opposite sides of said layer to explore the magnitude of the vertical versus radial epicyclic frequencies and confirm the anticipated scales of the observed frequencies. It also happens to recreate a 3:2 resonance ratio for the Keplerian angular frequencies at the ISCO, taken as the preferred radius for the boundary layer model.
A toy model was recreated and utilized to emulate the Alfven radius due to the accretion disk's innate magnetic field and explore how it serves as a disruption radius and impacts the accretion of mass and the effective inner edge of the disk. The simulations show that there is no significance deviation from the ISCO as an effective inner edge for the accretion disk due to the magnetospheric influence of the disk alone.
I also invoke a parameter to handle the coupling between the vertical and radial epicyclical frequencies and relate it to the pressure within the disk. I show the coupling is strongest at the equatorial plane where pressure is at its maximum value.
A model I utilize is a relativistic resonance model, combined with a helioseismological approach to explore the pulsation of the inner edge of the accretion disk that imparts the resonance of the accreting matter moving along the Kerr space-time orbits. The helioseismological model gives a characteristic frequency for small perturbations in the stellar matter within the atmosphere of a star. The diskoseismological model extends that principle to material within an accretion disk. I take it to the same extent that the QPO frequencies are due to small perturbations along the marginally stable circular orbit, in the vertical and radial directions and use it as a probe into the inner disk and what information it yields. The inner disk edge, per the model, is treated as a vibrating surface that yields the radial and vertical epicyclic frequencies as characteristic features of the vibration. The epicyclical frequencies found using the physical parameters of the model within the cusp layer inside the disk could explain the physical context of the phenomenon responsible for the creation of the QPOs. An approach within the diskoseismological model uses the cylindrical reference frame of a disk in terms of the distribution of mass in combination with the strong gravity of the central object and the Keplerian velocity and sonic speed to yield a natural resonance ratio of 3/2 as well.
The model can be used as a diagnostic tool to explore the physical phenomena of the material orbits and the disk itself. Most importantly, the model can be used to determine and constrain the ratio of spin to mass of the compact object itself. It yields new information as previously undetermined by any earlier model; the adiabatic index at a specific radius within the accretion disk, which serves to lend insight into the innate phenomena of accretion disks at large. It establishes what were previously unknown information, such as the mass density distribution at a specific radius and outward, the radius of influence in terms of the sonic radius, the accretion rate, and the temperature distribution at the same radius for the accretion disk, as all are dependent on the adiabatic index. In all previous literature, the adiabatic index is taken as an assumptive estimate, and the models build on that assumed value of the adiabatic index. This model allows us to obtain an actual value of the adiabatic index at the ISCO and use it as an establishing feature to refine models on for more physically realistic observations.
Ryan, James. "Measuring the energies and multiplicities of prompt gamma-ray emissions from neutron-induced fission of 235 U using the STEFF spectrometer". Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/measuring-the-energies-and-multiplicities-of-prompt-gammaray-emissions-from-neutroninduced-fission-of-235-u-using-the-steff-spectrometer(5fca332e-58ef-463f-96ba-99d87f0ecf44).html.
Texto completoSnowden, Mareena Robinson. "Nuclear warhead monitoring : a study of photon emissions from fission neutron interactions with high explosives as a tool in arms control verification". Thesis, Massachusetts Institute of Technology, 2017. http://hdl.handle.net/1721.1/113723.
Texto completoThis electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.
Cataloged from student-submitted PDF version of thesis.
Includes bibliographical references.
Since the signing of the Nuclear Nonproliferation Treaty, the technical community has been working to develop verification options that provide confidence in the reduction or elimination of nuclear warheads, while respecting countries' requirement of limited access to national secrets. This dissertation used a simplified open-source warhead model as a vehicle to investigate the use of secondary gammas, generated passively by neutron interactions inside high explosive (HE), as a signature for the presence of a warhead-like object. Analytical calculations were done to estimate the detectability of radiative capture and inelastic scatter emissions generated within the warhead model. Results showed the emission of gammas from nitrogen, between 5-7 MeV, to be detectable above background with dwell-times exceeding 90 minutes. These calculations motivated the systematic study of the signal experimentally using surrogate materials to represent the warhead's weapons-grade plutonium and HE. The experiment did not show the expected signals. This motivated a simulation of the mock-up experiment using the radiation transport code MCNP6 to help understand the observed results. The experimental and simulation data suggest that correlated backgrounds from neutron interactions with environmental materials dominate the signal. This finding helped provide a basis for understanding the feasibility and challenges to detecting this neutron-induced gamma signal. Three sets of pulse-height spectra have been analyzed: experimental spectra that looked at the effect of the HE surrogate on the overall detected counts; simulated spectra that helped to understand the underlying contributors to the observed experimental result; and a data-MCNP6 comparison that assessed the accuracy of the simulated results. Each set contributed to the quantification of detectability for the emissions of interest. The findings suggest the passive detection of the expected high-energy gamma signal is not feasible, unless backgrounds can be better controlled. The difficulty is attributed to low solid-angle coverage of the neutron source by the melamine explosive surrogate, and competing backgrounds produced by neutron-source interactions with surrounding materials. This thesis also examined the benefits and tradeoffs of this particular verification approach by investigating the non-technical context of the verification, such as the preferences of negotiators. The tradeoffs between confidence and intrusiveness highlight the need for technical verification solutions that span the diversity of options. Factors limiting the development of warhead verification systems, from the bias of researchers to issues of classification and sensitive geometries, were discussed.
by Mareena Robinson Snowden.
Ph. D.
Kundu, Anu. "Contribution of multipolar electromagnetic fields to the radio and high energy emission of pulsars". Thesis, Strasbourg, 2018. http://www.theses.fr/2018STRAE014/document.
Texto completoStudying the electromagnetic field around neutron stars is one of the vital methods to understand the physics of the pulsars. While major literature uses assumption of a standard centred dipolar electromagnetic field, recent studies have focused on including higher multipolar field components and have presented a more generalized picture for pulsars in which the magnetic dipole moment is shifted off from the centre of the star. This work discusses the consequences of an off centred rotating magnetic dipole in vacuum by showing various characteristic features of magnetic field lines and pulsar emission. A broadband spectrum study of pulsar radiation is also laid out by creating maps of different emission regions of pulsars distinguished on the basis of their frequency with the main aim of looking for the evolution of the pulse profile with frequency. The thesis presents all the above results accompanied by the necessary discussions to understand the theoretical models used and the details of the numerical methods applied
Klimek, Iwona. "Modelling and Measurements of MAST Neutron Emission". Doctoral thesis, Uppsala universitet, Tillämpad kärnfysik, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-282122.
Texto completoTaverna, Roberto. "Polarized emission from highly-magnetized neutron stars". Doctoral thesis, Università degli studi di Padova, 2016. http://hdl.handle.net/11577/3424483.
Texto completoLo studio delle magnetars, anomalous X-ray pulsars (AXPs) e soft gamma repeaters (SGRs), e delle X-ray Dim Isolated Neutron Stars (XDINSs) è di particolare rilevanza, dal momento che questi oggetti mostrano i più forti campi magnetici mai osservati nell'universo (10^13-10^15 G) e rappresentano i soli laboratori dove la fisica in presenza di campi magnetici così forti può essere testata. Fino ad ora, queste particolari stelle di neutroni sono state studiate attraverso misure spettroscopiche e di timing, che hanno portato a corroborare i modelli teorici formulati per spiegare la loro fenomenologia, come nel caso del "twisted magnetosphere'' model per le magnetars o dei diversi modelli di emissione superficiale per le XDINSs. Cionondimeno, questa analisi da sola non riesce a fornire informazioni complete. A questo riguardo, la polarimetria X può svelare un approccio completamente nuovo nello studio delle stelle di neutroni altamente magnetizzate. La radiazione emessa in presenza di forti campi magnetici, infatti, è attesa essere altamente polarizzata; le misure di polarizzazione forniscono due osservabili aggiuntivi, la frazione di polarizzazione lineare e l'angolo di polarizzazione, che possono determinare senza ambiguità i parametri dei modelli anche quando la sola analisi spettrale si dimostra insufficiente. Il segnale di polarizzazione che un osservatore riceve all'infinito, tuttavia, non coincide necessariamente con ciò che i modelli predicono per la polarizzazione alla superficie, a causa degli effetti dell'elettrodinamica quantistica nel vuoto fortemente magnetizzato attorno alla stella, accoppiato con la rotazione dei parametri di Stokes nel piano perpendicolare alla linea di vista, indotta dal campo magnetico non uniforme. In questa tesi presento i risultati dei codici numerici che ho sviluppato per simulare il pattern di polarizzazione, sia alla superficie che all'infinito, della radiazione emessa da stelle di neutroni isolate altamente magnetizzate, usando come modelli la luminosa AXP 1RXS 170849.0-400910 e la XDINS RX J1856.5-3754. Dimostrerò che le misure di polarizzazione possono effettivamente fornire informazioni cruciali sulle proprietà fisiche e geometriche di queste sorgenti, permettendo di testare direttamente i modelli teorici. Questo lavoro è inoltre rilevante in vista del lancio di polarimetri X di nuova generazione, attualmente in fase di sviluppo, come l'X-ray Imaging Polarimetry Explorer (XIPE). Per questa ragione, confronterò i modelli teorici con osservazioni simulate di XIPE, allo scopo di mostrare come le misure di polarizzazione possono essere utilizzate per estrarre i valori dei parametri relativi alla magnetosfera e gli angoli di vista.
Chietera, Andreina. "Angular correlations between fragments and neutrons in the spontaneous fissions of 252 Cf". Thesis, Strasbourg, 2015. http://www.theses.fr/2015STRAE048/document.
Texto completoThe subject of this thesis is to explore the neutron emission mechanisms in the fission process. In particular a long standing open question, the existence of a dynamical anisotropy in the centre of mass of the fission fragments and/or a possible scission neutron emission is explored. The thesis starts with an overview of the theoretical concepts on the fission process and on the neutron emission mechanisms. Also the necessity to conceive an appropriate analysis method is stressed when a very subtle mechanism is studied as various approximations and/or experimental biases not completely handled can hide the physical phenomena. In the presented work a huge effort was required to write a Monte Carlo procedure based on a coherent model for the spontaneous fission of 252Cf and to couple it with the devices exploited in the CORA3 experiment
GILIBERTI, ELIA. "ON NEUTRON STARS'CRUST BREAKING AND GRAVITATIONAL WAVES EMISSION". Doctoral thesis, Università degli Studi di Milano, 2020. http://hdl.handle.net/2434/704603.
Texto completoLibros sobre el tema "Neutron emissions"
Carpinteri, Alberto, Giuseppe Lacidogna y Amedeo Manuello, eds. Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2.
Texto completoNorbury, John W. Calculation of two-neutron multiplicity in photonuclear reactions. Hampton, Va: Langley Research Center, 1990.
Buscar texto completoInferences from Surface Thermal Emission of Young Neutron Stars. [New York, N.Y.?]: [publisher not identified], 2020.
Buscar texto completoJ, Hughes M., Cowell Michael, Hook Duncan R y British Museum. Dept. of Scientific Research., eds. Neutron activation and plasma emission spectrometric analysis in archaeology: Techniques and applications. London: British Museum, 1994.
Buscar texto completoHowarth, P. J. A. The JET neutron emission profile diagnostic: Data exploitation and the development of an upgraded version. Birmingham: University of Birmingham, 1994.
Buscar texto completoHartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1994.
Buscar texto completoHartmann, Dap. The Leiden/Dwingeloo survey of galactic neutral hydrogen. Leiden: Sterrewacht Leiden, 1995.
Buscar texto completoCiviš, Svatopluk, Ekaterina Zanozina, Adam Pastorek, Petr Kubelík, Martin Ferus y Ashok Chilukoti. Atomic Emission Spectra of Neutral Noble Gases in the Infrared Spectral Range. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-47352-5.
Texto completoNanda, Rea y SpringerLink (Online service), eds. High-Energy Emission from Pulsars and their Systems: Proceedings of the First Session of the Sant Cugat Forum on Astrophysics. Berlin, Heidelberg: Springer-Verlag Berlin Heidelberg, 2011.
Buscar texto completoR, Cominsky Lynn y United States. National Aeronautics and Space Administration., eds. ROSAT observations of the binary Be-star/radio pulsar PSR1259-63: Final technical report for NASA NAG 5-1684. [Washington, DC: National Aeronautics and Space Administration, 1994.
Buscar texto completoCapítulos de libros sobre el tema "Neutron emissions"
Manuello, A., R. Malvano, O. Borla, A. Palumbo y A. Carpinteri. "Neutron Emissions from Hydrodynamic Cavitation". En Fracture, Fatigue, Failure and Damage Evolution, Volume 8, 175–82. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-21611-9_22.
Texto completoBorla, Oscar, Giuseppe Lacidogna y Alberto Carpinteri. "Piezonuclear Neutron Emissions from Earthquakes and Volcanic Eruptions". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 135–51. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_10.
Texto completoCarpinteri, Alberto. "TeraHertz Phonons and Piezonuclear Reactions from Nano-scale Mechanical Instabilities". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 1–10. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_1.
Texto completoCarpinteri, Alberto, Giuseppe Lacidogna y Oscar Borla. "Is the Shroud of Turin in Relation to the Old Jerusalem Historical Earthquake?" En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 153–62. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_11.
Texto completoCarpinteri, Alberto y Amedeo Manuello. "Evolution and Fate of Chemical Elements in the Earth’s Crust, Ocean, and Atmosphere". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 163–81. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_12.
Texto completoCarpinteri, Alberto, Amedeo Manuello y Luca Negri. "Chemical Evolution in the Earth’s Mantle and Its Explanation Based on Piezonuclear Fission Reactions". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 183–96. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_13.
Texto completoCarpinteri, Alberto, Amedeo Manuello y Luca Negri. "Piezonuclear Fission Reactions Triggered by Fracture and Turbulence in the Rocky and Gaseous Planets of the Solar System". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 197–218. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_14.
Texto completoCook, Norman D., Amedeo Manuello, Diego Veneziano y Alberto Carpinteri. "Piezonuclear Fission Reactions Simulated by the Lattice Model of the Atomic Nucleus". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 219–35. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_15.
Texto completoNiccolini, Gianni, Oscar Borla, Giuseppe Lacidogna y Alberto Carpinteri. "Correlated Fracture Precursors in Rocks and Cement-Based Materials Under Stress". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 237–48. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_16.
Texto completoAccornero, Federico, Stefano Invernizzi, Giuseppe Lacidogna y Alberto Carpinteri. "The Sacred Mountain of Varallo Renaissance Complex in Italy: Damage Analysis of Decorated Surfaces and Structural Supports". En Acoustic, Electromagnetic, Neutron Emissions from Fracture and Earthquakes, 249–64. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-16955-2_17.
Texto completoActas de conferencias sobre el tema "Neutron emissions"
KEENEY, F. W., S. E. JONES, A. C. JOHNSON, P. L. HAGELSTEIN, G. HUBLER, D. B. BUEHLER, F. E. CECIL, M. R. SCOTT y J. E. ELLSWORTH. "NEUTRON EMISSIONS FROM DEUTERIDED METALS". En Proceedings of the 10th International Conference on Cold Fusion. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701510_0045.
Texto completoCelik, C., R. O’Mara y W. Wieselquist. "Monte Carlo Uncertainty Quantification in UF6 Cylinder Neutron Emissions". En Tranactions - 2019 Winter Meeting. AMNS, 2019. http://dx.doi.org/10.13182/t31282.
Texto completoGupta, Sanjib S., A. Heger, P. Möller, T. Kawano, Jutta Escher, Frank S. Dietrich, Toshihiko Kawano y Ian J. Thompson. "Electron Capture-delayed neutron-emissions in neutron star crust simulations using a Hauser-Feshbach model". En COMPOUND-NUCLEAR REACTIONS AND RELATED TOPICS: Proceedings of the 2007 International Workshop on Compound-Nuclear Reactions and Related Topics - CNR∗ 2007. AIP, 2008. http://dx.doi.org/10.1063/1.2920735.
Texto completoJones, S. E., D. Bennion, D. Buehler, J. B. Czirr, D. L. Decker, J. Harb, R. Hunter et al. "In quest of a trigger mechanism for neutron emissions from deuterium/solid systems". En Anomalous nuclear effects in deuterium/solid systems. AIP, 1991. http://dx.doi.org/10.1063/1.40694.
Texto completoGolubnichyi, P. I., A. D. Philonenko, A. A. Tsaric, V. V. Kuzminov, B. V. Pritichenko, G. I. Merzon y V. A. Tsarev. "Recording of neutron and acoustic emissions from palladium target in a low background underground experiment". En Anomalous nuclear effects in deuterium/solid systems. AIP, 1991. http://dx.doi.org/10.1063/1.40715.
Texto completoJeong, Han Koo y Soo Hyoung Kim. "Effect of Marine Nuclear Reactor Environment to Ship’s Structural Responses". En ASME 2021 40th International Conference on Ocean, Offshore and Arctic Engineering. American Society of Mechanical Engineers, 2021. http://dx.doi.org/10.1115/omae2021-62600.
Texto completoYAKOVLEV, D. G., M. E. GUSAKOV, A. D. KAMINKER y A. Y. POTEKHIN. "NEUTRINO EMISSION FROM NEUTRON STARS". En Proceedings of the Carpathian Summer School of Physics 2005. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812772862_0024.
Texto completoAcevedo, Wilson, Luis Gaitan, Andrés Julián Aristizábal y Daniel Ospina. "Study of the effect on greenhouse gas emissions of vehicles powered by hydrogen generators". En XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY. AIP Publishing, 2019. http://dx.doi.org/10.1063/1.5116941.
Texto completoAndriyash, A. V. "Investigation of Neutron Emissions from D(d,n)3He and T(d,n)4He Reactions in a 10 TW Picosecond Laser Facility SOKOL-P". En ZABABAKHIN SCIENTIFIC TALKS - 2005: International Conference on High Energy Density Physics. AIP, 2006. http://dx.doi.org/10.1063/1.2337173.
Texto completoFrankfurt, Leonid, Mark Strikman, Sigfrido Boffi, Claudio Ciofi degli Atti, Mauro Giannini y Daniele Treleani. "Short-range nucleon correlations and neutrino emission by neutron stars". En SIXTH INTERNATIONAL CONFERENCE ON PERSPECTIVES IN HADRONIC PHYSICS. AIP, 2008. http://dx.doi.org/10.1063/1.3013048.
Texto completoInformes sobre el tema "Neutron emissions"
Kocharov, L. G., Jeongwoo W. Lee, H. Zirin, G. A. Kovaltsov y I. G. Usoskin. Neutron and Electromagnetic Emissions During the 1990 May 24 Solar Flare,. Fort Belvoir, VA: Defense Technical Information Center, diciembre de 1996. http://dx.doi.org/10.21236/ada319276.
Texto completoEpstein, R. I., B. C. Edwards y T. J. Haines. Neutron star evolution and emission. Office of Scientific and Technical Information (OSTI), agosto de 1997. http://dx.doi.org/10.2172/515633.
Texto completoStrachan, J., M. Bell, M. Bitter, R. Budny, R. Hawryluk, K. Hill, H. Hsuan et al. Neutron emission from TFTR supershots. Office of Scientific and Technical Information (OSTI), octubre de 1992. http://dx.doi.org/10.2172/6946572.
Texto completoStrachan, J. D., M. G. Bell, M. Bitter, R. Budny, R. Hawryluk, K. W. Hill, H. Hsuan et al. Neutron emission from TFTR supershots. Office of Scientific and Technical Information (OSTI), octubre de 1992. http://dx.doi.org/10.2172/10184799.
Texto completoLitz, Marc, Christopher Waits y Jennifer Mullins. Neutron-Activated Gamma-Emission: Technology Review. Fort Belvoir, VA: Defense Technical Information Center, enero de 2012. http://dx.doi.org/10.21236/ada554870.
Texto completoPark, H. K., M. G. Bell, W. M. Tang, G. Taylor y M. Yamada. Role of neutral-beam fueling profile in energy confinement and neutron emission on TFTR. Office of Scientific and Technical Information (OSTI), octubre de 1993. http://dx.doi.org/10.2172/10189872.
Texto completoShores, Erik Frederick. Tabulated Neutron Emission Rates for Plutonium Oxide. Office of Scientific and Technical Information (OSTI), julio de 2017. http://dx.doi.org/10.2172/1372807.
Texto completoPellarin, D. J. (a, n) Neutron Emission from DWPF Glass. Office of Scientific and Technical Information (OSTI), marzo de 2001. http://dx.doi.org/10.2172/780500.
Texto completoGoldberg, E., L. F. Hansen, R. J. Howerton, T. T. Komoto y B. A. Pohl. HOTSPUR: Neutron and gamma-ray emission from the transport of 14 MeV neutrons through H/sub 2/O. Office of Scientific and Technical Information (OSTI), mayo de 1987. http://dx.doi.org/10.2172/6319434.
Texto completoMadland, D. G. Post-scission fission theory: Neutron emission in fission. Office of Scientific and Technical Information (OSTI), noviembre de 1997. http://dx.doi.org/10.2172/548904.
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