Готові списки джерел за темами / High-energy nuclear physic

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Автор: Grafiati
Опубліковано: 14 березня 2023

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Статті в журналах з теми "High-energy nuclear physic"

1

Heil, Werner. "From nuclear physic to NMR tomography." Nuclear Physics News 12, no. 3 (January 2002): 30–34. http://dx.doi.org/10.1080/10506890208232682.

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2

Vogt, R. "Physic of the nucleon sea quark distributions." Progress in Particle and Nuclear Physics 45 (January 2000): S105—S169. http://dx.doi.org/10.1016/s0146-6410(00)90012-7.

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3

Zhao, L., and C. L. Liu. "A Multi-Physic Field Lifetime Evaluation Formula for Insulators Under Pulsed Field and Mechanical Stress." IEEE Transactions on Plasma Science 49, no. 12 (December 2021): 3913–18. http://dx.doi.org/10.1109/tps.2021.3125787.

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4

ARDID, M., J. RAMIS, V. ESPINOSA, J. A. MARTÍNEZ-MORA, F. CAMARENA, J. ALBA, and V. SANCHEZ-MORCILLO. "FIRST ACTIVITIES IN ACOUSTIC DETECTION OF PARTICLES IN UPV." International Journal of Modern Physics A 21, supp01 (July 2006): 137–41. http://dx.doi.org/10.1142/s0217751x06033519.

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The first activities related to acoustic detection of particles by DISAO research group in the Univesitat Politècnica de València are described. We are applying some techniques from physic, engineering and oceanographic acoustics to face the high energy neutrino underwater acoustic detection challenge. The work is focused mainly in two topics: design, characterization and calibration of hydrophones, and simulation of the propagation of the signal in the sea. We present also some examples for these two topics: piezoelectric modelling and transducer simulation, calibration of hydrophones using MLS signals, and evaluation of the contribution of the sea surface noise to the deep water noise in the Mediterranean Sea by means of simulations of propagation of sound.
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5

KWEON, MinJung, Dongho MOON, Sungtae CHO, and Byungsik HONG. "High Energy Nuclear Physics." Physics and High Technology 28, no. 1/2 (February 28, 2019): 2–9. http://dx.doi.org/10.3938/phit.28.001.

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6

Shen, W. Q. "High-energy nuclear physics in China." Journal of Physics G: Nuclear and Particle Physics 34, no. 8 (July 4, 2007): S173—S179. http://dx.doi.org/10.1088/0954-3899/34/8/s01.

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7

Sun, Hancheng, and Donghai Zhang. "Nuclear emulsion and high-energy physics." Radiation Measurements 43 (August 2008): S139—S143. http://dx.doi.org/10.1016/j.radmeas.2008.04.019.

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8

Fares, Reine, David Castro Cruz, Evelyne Foerster, Fernando Lopez-Caballero, and Filippo Gatti. "Coupling spectral and Finite Element methods for 3D physic-based seismic analysis from fault to structure: Application to the Cadarache site in France." Nuclear Engineering and Design 397 (October 2022): 111954. http://dx.doi.org/10.1016/j.nucengdes.2022.111954.

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9

Gobet, F., C. Plaisir, F. Hannachi, M. Tarisien, T. Bonnet, M. Versteegen, M. M. Aléonard, G. Gosselin, V. Méot, and P. Morel. "Nuclear physics studies using high energy lasers." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 653, no. 1 (October 2011): 80–83. http://dx.doi.org/10.1016/j.nima.2011.01.106.

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10

Newman, Harvey B. "Networking for High Energy and Nuclear Physics." Computer Physics Communications 177, no. 1-2 (July 2007): 224–30. http://dx.doi.org/10.1016/j.cpc.2007.02.002.

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Дисертації з теми "High-energy nuclear physic"

1

Szabo, Anthony Paul. "High energy emissions for astrophysical objects." Title page, contents and abstract only, 1992. http://web4.library.adelaide.edu.au/theses/09PH/09phs996.pdf.

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2

Frederiksen, Joorgen Segerlund. "Theoretical studies in high energy physics and atmospheric dynamics /." Title page, introduction and contents only, 1987. http://web4.library.adelaide.edu.au/theses/09SD/09sdf852.pdf.

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3

Kvasnikova, Ioulia. "Mesonic sources of dileptons in ultrarelativistic nuclear collisions." Thesis, McGill University, 2001. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=37753.

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In this work thermal dilepton production from a hot medium created in heavy ion collision is studied. Using an effective Lagrangian technique for particle decays and annihilations, a complete method for calculation of the lepton pair production rate is developed. The importance of axial vector meson contributions to the dilepton spectrum is analyzed. Different effective Lagrangians for the a1rhopi interaction are considered, and a new form of b1o(&phis;)pi effective Lagrangian is introduced.
A systematic study of light meson contributions is performed. The most significant decay and reaction contributions are calculated and summed for low and intermediate invariant mass dileptons. The calculated dilepton rate is compared to that obtained using spectral functions extracted from data, and it is shown that the chosen set of mesonic reactions and decays accounts for all significant contributions to the thermal dilepton emission.
A hydrodynamic approach to the space-time evolution of the hot medium formed as a result of a central heavy ion collision at ultra-relativistic energies is considered. A theoretical curve of intermediate invariant mass dilepton spectrum is computed and compared to the NA50 data from central Pb(158 AGeV)+Pb collisions. Experimental acceptance cuts are accounted for. Drell-Yan processes are considered as well. We find that our thermal dileptons account for the intermediate mass excess observed by the NA50 Collaboration. We see no need to invoke charm enhancement. Predictions for the future experiments at RHIC and are made.
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4

Eggers, Hans Christoph. "Intermittency, moments and correlations in distributions of particles created in high-energy collisions." Diss., The University of Arizona, 1991. http://hdl.handle.net/10150/185422.

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Intermittency, as introduced into multiparticle production by Bialas and Peschanski, has become a fruitful and rapidly growing industry. The original concept of intermittency in the form of the Alpha model is discussed in detail and suggestions for extensions are made. We analyze the factorial moments measured by different experimental collaborations in terms of their nontrivial many-particle correlations, the cumulants. A large fraction of measured moments is shown to originate in two-particle correlations. The validity of the Linked Pair ansatz is tested and found to be acceptable to fourth order for hadronic collisions but uncertain for nuclear collisions. A cumulant decomposition for bin-bin correlations is derived, and a general formalism is developed for treating correlations of particle distributions consisting of several distinct populations, such as particles of different charge.
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5

Bourque, François-Alex. "Electromagnetic signature of early gluon populations in ultrarelativistic nuclear collisions." Thesis, McGill University, 2002. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=78326.

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We first present a brief overview of the quark-gluon plasma (QGP) and its possible production in a heavy ion collision. Equilibrium quantum field theory is then outlined as a tool to study QGP. With this, we investigate the consequence of a finite charge density plasma through the breaking of Furry's theorem. In particular, we calculate the dilepton differential production rate for one of the simplest medium-induced processes: 2g → ll¯. We show that this effect is sub-dominant to the leading tree-level qq¯ → ll¯.
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6

Wang, Yongjiang. "Aspects of pion propagation in hot and dense nuclear matter." Thesis, McGill University, 1991. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=60494.

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Some important aspects of pion propagation in hot and dense nuclear matter are investigated by considering the dominant p-wave pion nucleon interaction including the $ Delta$-isobar channel. We find that for zero temperature nuclear mater, the static approximation in the computation of the pion branch dispersion relation is not adequate in general. In the finite temperature nuclear matter up to T = 50MeV, the pion propagation does not change much comparing to that in the zero temperature medium, but the pion absorption through the first order pion-nucleon interaction, on the other hand, increases significantly as the temperature goes up. We also give a formula to determine the critical nuclear matter density $ rho sb{c}$ and when $ rho > rho sb{c}$ is satisfied, a minimum exists in the corresponding pion branch.
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7

Abrahamyan, Tigran. "High energy three-body breakup of three-nucleon systems." FIU Digital Commons, 2007. http://digitalcommons.fiu.edu/etd/1107.

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The main goal of this dissertation was to study two- and three-nucleon Short Range Correlations (SRCs) in high energy three-body breakup of 3He nucleus in 3He(e, e'NN)N reaction. SRCs are characterized by quantum fluctuations in nuclei during which constituent nucleons partially overlap with each other. A theoretical framework is developed within the Generalized Eikonal Approximation (GEA) which upgrades existing medium-energy methods that are inapplicable for high momentum and energy transfer reactions. High momentum and energy transfer is required to provide sufficient resolution for probing SRCs. GEA is a covariant theory which is formulated through the effective Feynman diagrammatic rules. It allows self-consistent calculation of single and double re-scatterings amplitudes which are present in three-body breakup processes. The calculations were carried out in detail and the analytical result for the differential cross section of 3He(e, e'NN)Nreaction was derived in a form applicable for programming and numerical calculations. The corresponding computer code has been developed and the results of computation were compared to the published experimental data, showing satisfactory agreement for a wide range of values of missing momenta. In addition to the high energy approximation this study exploited the exclusive nature of the process under investigation to gain more information about the SRCs. The description of the exclusive 3He(e, e'NN)N reaction has been done using the formalism of the nuclear decay function, which is a practically unexplored quantity and is related to the conventional spectral function through the integration of the phase space of the recoil nucleons. Detailed investigation showed that the decay function clearly exhibits the main features of two- and three-nucleon correlations. Four highly practical types of SRCs in 3He nucleus were discussed in great detail for different orders of the final state re-interactions using the decay function as an unique identifying tool. The overall conclusion in this dissertation suggests that the investigation of the decay function opens up a completely new venue in studies of short range nuclear properties.
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8

Biehl, Daniel. "Nuclear Cascades and Neutrino Production in the Sources of Ultra-High Energy Cosmic Ray Nuclei." Doctoral thesis, Humboldt-Universität zu Berlin, 2019. http://dx.doi.org/10.18452/20448.

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Der Ursprung ultra-hochenergetischer kosmischer Strahlung (UHECRs) ist eine der wichtigsten offenen Fragen der Astrophysik. Gammastrahlenblitze (GRBs) galten als potentielle Quellen, da sie zu den energetischsten Ereignissen im Universum zählen. Konventionelle Szenarien sind jedoch durch Neutrinodaten stark eingeschränkt. Außerdem weisen Messungen der chemischen Zusammensetzung kosmischer Strahlen auf schwere Kerne hin, welche in zu dichten Strahlungsfeldern disintegrieren würden. Um dieses Dilemma zu umgehen deuten neue Studien auf versteckte Beschleuniger hin, welche schwer zu detektieren sind. In dieser Dissertation präsentieren wir neue Ansätze um nukleare Prozesse in astrophysikalischen Quellen effizient und selbstkonsistent zu berechnen. Wir quantifizieren diese Wechselwirkungen anhand der nuklearen Kaskade, welche die Disintegration schwerer Kerne in leichtere Fragmente beschreibt. Auch in umfassenden Modellen, wie sie in dieser Arbeit entwickelt werden, sind GRBs durch Neutrinodaten unter Druck. Dennoch zeigen wir, dass eine Population von GRBs niedriger Luminosität konsistent mit derzeitigen Messungen ist und zugleich auch das Spektrum und die Zusammensetzung kosmischer Strahlung über den Knöchel hinweg sowie Neutrinodaten beschreiben kann. Aus unserer Prozedur können wir zusätzlich weitere Quelleneigenschaften wie die baryonische Ladung oder die Ereignisrate bestimmen. Wir zeigen weiter, dass auch von schwarzen Löchern zerrissene Sterne mögliche Kandidaten eines gemeinsamen Ursprungs der gemessenen kosmischen Strahlung und PeV-Neutrinos sind. Sie können jedoch durch kosmogenische Neutrinos von LLGRBs abgegrenzt werden. Schließlich wenden wir unser Modell auf das Gravitationswellenereignis GW170817 an. Wir zeigen für verschiedene Jet-Szenarien, dass der erwartete Neutrinofluss weit unter der Sensitivität derzeitiger Instrumente liegt. Dennoch könnten verschmelzende Neutronensterne die kosmische Strahlung unterhalb des Knöchels erklären.
The origin of Ultra-High Energy Cosmic Rays (UHECRs) is still one of the most important open questions in astrophysics. Gamma-Ray Bursts (GRBs) were considered as potential sources as they are among the most energetic events known in the Universe. However, conventional GRB scenarios are strongly constrained by astrophysical neutrino data. In addition, cosmic ray composition measurements indicate the presence of heavy nuclei, which would disintegrate if the radiation fields in the source were too dense. In order to circumvent this dilemma, recent studies point towards hidden accelerators, which are intrinsically hard to detect. In this dissertation, we present novel approaches to efficiently and self-consistently calculate the nuclear processes in astrophysical sources. We quantify these interactions by means of the nuclear cascade, which describes the subsequent disintegration of heavy nuclei into lighter fragments. Even in sophisticated source-propagation models, as the ones developed in this thesis, conventional GRBs are in tension with neutrino data. However, we demonstrate that a population of low-luminosity GRBs is not only consistent with current constraints, but can even describe the UHECR spectrum and composition across the ankle as well as neutrino data simultaneously. From our fitting procedure we can further constrain certain source properties, such as the baryonic loading and the event rate. Furthermore, we show that stars disrupted by black holes are viable candidates for a simultaneous description of cosmic ray and PeV neutrino data too. However, they can be discriminated from LLGRBs by cosmogenic neutrinos. Finally, we apply our model to GW170817. We show for different jet scenarios that the expected neutrino flux is orders of magnitude below the sensitivity of current instruments. Nevertheless, binary neutron star mergers could in principle support cosmic rays below the ankle.
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9

Zarkadoula, Evangelia. "Modelling of high-energy radiation damage in materials relevant to nuclear and fusion energy." Thesis, Queen Mary, University of London, 2013. http://qmro.qmul.ac.uk/xmlui/handle/123456789/8607.

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The objective through my PhD has been to investigate radiation damage effects in materials related to fusion and to safe encapsulation of nuclear waste, using Molecular Dynamics (MD) methods. Particularly, using MD, we acquire essential information about the multi-scale phenomena that take place during irradiation of materials, and gain access at length and time-scales not possible to access experimentally. Computer simulations provide information at the microscopic level, acting as a bridge to the experimental observations and giving insights into processes that take place at small time and length-scales. The increasing computer capabilities in combination with recently developed scalable codes, and the availability of realistic potentials set the stage to perform large scale simulations, approaching phenomena that take place at the atomistic and mesoscopic scale (fractions of m for the first time) in a more realistic way. High-energy radiation damage effects have not been studied previously, yet it is important to simulate and reveal information about the properties of the materials under extreme irradiation conditions. Large scale MD simulations provide a detailed description of microstructural changes. Understanding of the primary stage of damage and short term annealing (scale of tens of picoseconds) will lead to better understanding of the materials properties, best possible long-term use of the materials and, importantly, new routes of optimization of their use. Systems of interest in my research are candidate fusion reactor structural materials (iron and tungsten) and materials related to the radioactive waste management (zirconia). High-energy events require large simulation box length in order for the damage to be contained in the system. This was a limitation for previous simulations, which was recently shifted with my radiation damage MD simulations. For the first time high-energy radiation damage effects were simulated, approaching new energy and length scales, giving a more realistic view of processes related to fusion and to high-energy ion irradiation of material.
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10

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

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Книги з теми "High-energy nuclear physic"

1

International, Triangle Workshop JINR-CERN-IHEP (1st 1990 Dubna Chekhovskiĭ raĭon R. S. F. S. R. ). Standard model and beyond: From LEP to UNK and LHC : First International Conference Workshop JINR-CERN-IHEP, 1-5 October 1990, Dubna, USSR. Singapore: World Scientific, 1991.

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2

Joint International Lepton-Photon Symposium & Europhysics Conference on High Energy Physics (1991 Geneva, Switzerland). Proceedings of the Joint International Lepton-Photon Symposium & Europhysics Conference on High Energy Physics, Geneva, Switzerland, 25 July-1 August 1991. Edited by Hegarty S, Potter K, Quercigh E, European Physical Society, International Union of Pure and Applied Physics., and European Council for Nuclear Research. Singapore: World Scientific, 1992.

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3

S, Hegarty, Potter K, Quercigh E, European Physical Society, International Union of Pure and Applied Physics., and European Council for Nuclear Research., eds. Proceedings of the Joint International Lepton-Photon Symposium & Europhysics Conference on High Energy Physics, Geneva, Switzerland, 25 July-1 August 1991. Singapore: World Scientific, 1992.

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4

K, Ellis R., Hill C. T, and Lykken J. D, eds. Perspectives in the standard model: Proceedings of the Theoretical Advanced Study Institute in Elementary Particle Physics, Boulder, Colorado, 2-28 June, 1991. Singapore: World Scientific, 1992.

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5

1943-, Soper Davison E., ed. QCD & beyond: Proceedings of the Theoretical Advanced Study Institute in Elementary Particle Physics (TASI '95), Boulder, Colorado, USA, 4-30 June 1995. Singapore: World Scientific, 1996.

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6

G, Diambrini-Palazzi, and International Conference on "Phenomenology of Unification from Present to Future" (1st : 1994 : Rome, Italy), eds. Phenomenology of unification from the present to future: 23-26 March, 1994, Roma. Singapore: World Scientific, 1994.

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7

A, Greenwood D., ed. An introduction to the standard model of particle physics. Cambridge: Cambridge University Press, 1998.

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8

High energy astrophysics. 3rd ed. Cambridge: Cambridge University Press, 2011.

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9

Perkins, Donald H. Introduction to high energy physics. 4th ed. Cambridge: Cambridge University Press, 2000.

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10

Perkins, Donald H. Introduction to high energy physics. 3rd ed. Menlo Park, Calif: Addison-Wesley Pub. Co., 1987.

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Частини книг з теми "High-energy nuclear physic"

1

Plasil, F. "High Energy Nuclear Collisions." In International Europhysics Conference on High Energy Physics, 166–75. Berlin, Heidelberg: Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/978-3-642-59982-8_14.

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2

Drukarev, Evgeny G., and Aleksandr I. Mikhailov. "Nuclear Transitions and the Electron Shell." In High-Energy Atomic Physics, 345–82. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-32736-5_12.

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3

Yokosawa, A. "Structures in the Nucleon-Nucleon System." In High Energy Spin Physics, 526–29. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-86995-2_63.

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4

Liburg, M., and V. Matafonov. "A Remark on Nuclear Spin-Lattice Relaxation." In High Energy Spin Physics, 376–77. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-76661-9_74.

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5

Grosa, Fabrizio. "Introduction to High-Energy Nuclear Physics." In Springer Theses, 1–20. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-71131-3_1.

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6

Ramsey, G. P. "Spin Observables for Nucleon-Nucleon Elastic Scattering at Large Momentum Transfer." In High Energy Spin Physics, 476–79. Berlin, Heidelberg: Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-642-86995-2_52.

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7

Sidharth, B. G. "Ultra High Energy Neutrons and Other Fermions." In Nuclear Physics: Present and Future, 297–301. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10199-6_28.

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8

Hasse, Rainer W., and William D. Myers. "Medium- and High-Energy Nuclear Collisions." In Geometrical Relationships of Macroscopic Nuclear Physics, 119–25. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-83017-4_11.

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9

Martin, Joseph D. "Nuclear, High Energy, and Solid State Physics." In A Companion to the History of American Science, 186–97. Chichester, UK: John Wiley & Sons, Ltd, 2015. http://dx.doi.org/10.1002/9781119072218.ch15.

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10

Demtröder, Wolfgang. "Applications of Nuclear- and High Energy Physics." In Undergraduate Lecture Notes in Physics, 213–50. Cham: Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-58313-2_8.

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Тези доповідей конференцій з теми "High-energy nuclear physic"

1

Paul, Biswarup. "$\psi$(2S) production and nuclear modification factor in nucleus-nucleus collisions with ALICE." In 41st International Conference on High Energy physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.414.0445.

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2

Cerulli, Riccardo. "NUCLEUS: cryogenic calorimeters to detect coherent nuclear scattering of reactor antineutrinos." In 41st International Conference on High Energy physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.414.0589.

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3

Doglioni, Caterina. "Synergies between astroparticle, particle and nuclear physics." In European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.364.0686.

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4

Galati, Giuliana. "Directional Dark Matter Search with Nuclear Emulsion." In European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.364.0083.

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5

Bodek, Arie, and Tejin Cai. "Nuclear Potential of Final State Nucleons and Nucleons Plus Single Pions in Lepton Nucleus Scattering." In 40th International Conference on High Energy physics. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.390.0117.

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6

YU, Ji Young, Karol Kovarik, Ingo Schienbein, Fred Olness, Cynthia Keppel, Jorge G. Morfin, Joseph Francis Owens, and Tzvetalina STAVREVA. "Nuclear corrections in neutrino--nucleus DIS and their compatibility with global NPDF analysis." In XXIst International Europhysics Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2012. http://dx.doi.org/10.22323/1.134.0289.

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7

Pal, MK, D. Bhaumik, K. Kar, JN De, and BB Baliga. "MEDIUM AND HIGH ENERGY NUCLEAR PHYSICS." In Conference. WORLD SCIENTIFIC, 1993. http://dx.doi.org/10.1142/9789814537155.

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8

Ajaz, Muhammad, Mais Kazim Suleymanov, and Kamal Hussain Khan. "Nuclear transparency effect in proton and deuteron induced interaction with carbon nuclei." In XXI International Baldin Seminar on High Energy Physics Problems. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.173.0052.

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9

Mamatkulov, Kahramon Ziyadullayevich. "Fragmentation of relativistic $^{10}$C radioactive nuclei in a track nuclear emulsion." In XXII International Baldin Seminar on High Energy Physics Problems. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.225.0128.

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10

Baldin, A. M., V. V. Burov, and L. P. Kaptari. "RELATIVISTIC NUCLEAR PHYSICS & QUANTUM CHROMODYNAMICS." In Xth International Seminar on High Energy Physics Problems. WORLD SCIENTIFIC, 1991. http://dx.doi.org/10.1142/9789814538367.

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Звіти організацій з теми "High-energy nuclear physic"

1

Riley, Mark, and Akis Pipidis. The Mechanical Analogue of the "Backbending" Phenomenon in Nuclear-structure Physics. Florida State University, May 2008. http://dx.doi.org/10.33009/fsu_physics-backbending.

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Анотація:
This short pedagogical movie illustrates an effect in nuclear physics called backbending which was first observed in the study of the rotational behavior of rapidly rotating rare-earth nuclei in Stockholm, Sweden in 1971. The video contains a mechanical analog utilizing rare-earth magnets and rotating gyroscopes on a turntable along with some historic spectra and papers associated with this landmark discovery together with its explanation in terms of the Coriolis induced uncoupling and rotational alignment of a specific pair of particles occupying high-j intruder orbitals. Thus backbending represents a crossing in energy of the groundstate, or vacuum, rotational band by another band which has two unpaired high-j nucleons (two quasi-particles) with their individual angular momenta aligned with the rotation axis of the rapidly rotating nucleus. Backbending was a major surprise which pushed the field of nuclear structure physics forward but which is now sufficiently well understood that it can be used as a precision spectroscopic tool providing useful insight for example, into nuclear pairing correlations and changes in the latter due to blocking effects and quasi-particle seniority, nuclear deformation, the excited configurations of particular rotational structures and the placement of proton and neutron intruder orbitals at the Fermi surface.
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2

Vary, J. P. Intermediate/high energy nuclear physics. Office of Scientific and Technical Information (OSTI), January 1992. http://dx.doi.org/10.2172/5083299.

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3

Dart, Eli, Lothar Bauerdick, Greg Bell, Leandro Ciuffo, Sridhara Dasu, Vince Dattoria, Kaushik De, et al. High Energy Physics and Nuclear Physics Network Requirements. Office of Scientific and Technical Information (OSTI), March 2014. http://dx.doi.org/10.2172/1134243.

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4

Hwa, Rudolph C. Physics of Nuclear Collisions at High Energy. Office of Scientific and Technical Information (OSTI), May 2012. http://dx.doi.org/10.2172/1159986.

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5

Milner, Richard. Laboratory for Nuclear Science. High Energy Physics Program. Office of Scientific and Technical Information (OSTI), July 2014. http://dx.doi.org/10.2172/1214329.

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6

Hoffmann, Gerald W., and Christina Markert. Studies in High Energy Heavy Ion Nuclear Physics. Office of Scientific and Technical Information (OSTI), September 2016. http://dx.doi.org/10.2172/1324626.

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7

Vary, J. P. Intermediate/high energy nuclear physics. [Iowa State Univ. , Ames, Iowa]. Office of Scientific and Technical Information (OSTI), January 1992. http://dx.doi.org/10.2172/6703215.

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8

Schalk, T. 2003 Conference for Computing in High Energy and Nuclear Physics. Office of Scientific and Technical Information (OSTI), October 2003. http://dx.doi.org/10.2172/826552.

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9

Rafelski, Johann. Research in Theoretical High Energy Nuclear Physics at the University of Arizona. Office of Scientific and Technical Information (OSTI), March 2016. http://dx.doi.org/10.2172/1244424.

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10

Tang, L. Selected problems in nuclear/high energy physics: Experimental hypernuclear physics, muon rare decay, and development of new detector system applicable to nuclear/high energy physics experiments. Final close-out report, June 1, 1994--May 31, 1997. Office of Scientific and Technical Information (OSTI), August 1998. http://dx.doi.org/10.2172/666139.

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