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Добірка наукової літератури з теми "Light nuclei spectrum"

Автор: Grafiati

Опубліковано: 11 березня 2023

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Статті в журналах з теми "Light nuclei spectrum"

1

VARY, JAMES P., PIETER MARIS, and ANDREY SHIROKOV. "AB INITIO NO CORE METHODS: APPLICATIONS TO LIGHT NUCLEI." International Journal of Modern Physics E 17, supp01 (2008): 109–21. http://dx.doi.org/10.1142/s0218301308011793.

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We introduce a no-core full configuration (NCFC) approach and present results for 4 He , 12 C , 14 F and some other nuclei with the realistic NN interaction, JISP16. We obtain ground state energies and their uncertainties through exponential extrapolations that we demonstrate are reliable in 4 He where fully converged results are obtained. We find 12 C is overbound by 1.7 MeV and we predict the yet-to-be-measured binding energy of 14 F to be 70.2±3.5 MeV. The extrapolated spectrum of 14 F is in reasonable agreement with known features of the 14 B spectrum. Distinctions are drawn between this a

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2

Morigaki, Kazuo. "Light-induced defect creation processes and light-induced defects in hydrogenated amorphous silicon." European Physical Journal Applied Physics 90, no. 2 (2020): 20101. http://dx.doi.org/10.1051/epjap/2020190257.

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We have proposed a model of light-induced defect creation processes and light-induced defects. Recently, important results using pulsed electron-nuclear double resonance (ENDOR) by Fehr et al. [M. Fehr, A. Schnegg, C. Teutloff, R. Bittl, O. Astakhov, F. Finger, B. Rech, K. Lips, Phys. Status Solidi A 207, 552 (2010)] have been reported, so that these results are interpreted on the basis of our model. Fehr et al. have observed ENDOR signals due to hydrogen nuclei distributed around a dangling bond. The ENDOR spectra due to hydrogen nuclei being located with distance of r from the dangling bond

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3

Kalmykov, N. N., G. V. Kulikov, V. P. Sulakov, Yu A. Fomin, and V. N. Kalmykov. "On the energy spectrum of light nuclei in primary cosmic rays." Bulletin of the Russian Academy of Sciences: Physics 73, no. 5 (2009): 558–60. http://dx.doi.org/10.3103/s1062873809050074.

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4

Qinghua Wang, 王清华, 李振华 Zhenhua Li, 来建成 Jiancheng Lai, and 贺安之 Anzhi He. "Fourier analysis of elastic light scattering spectrum of epithelial cell nuclei." Chinese Optics Letters 8, no. 3 (2010): 278–81. http://dx.doi.org/10.3788/col20100803.0278.

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5

Mazur, I. A., A. M. Shirokov, A. I. Mazur, et al. "Description of Continuum Spectrum States of Light Nuclei in the Shell Model." Physics of Particles and Nuclei 50, no. 5 (2019): 537–43. http://dx.doi.org/10.1134/s1063779619050186.

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6

Pahlavani, M. R., and R. Morad. "Application of AdS/CFT in Nuclear Physics." Advances in High Energy Physics 2014 (2014): 1–19. http://dx.doi.org/10.1155/2014/863268.

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Анотація:

We review some recent progress in studying the nuclear physics especially nucleon-nucleon (NN) force within the gauge-gravity duality, in context of noncritical string theory. Our main focus is on the holographic QCD model based on the AdS6background. We explain the noncritical holography model and obtain the vector-meson spectrum and pion decay constant. Also, we study the NN interaction in this frame and calculate the nucleonmeson coupling constants. A further topic covered is a toy model for calculating the light nuclei potential. In particular, we calculate the light nuclei binding energie

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7

VAAGEN, J. S., B. V. DANILIN, and S. N. ERSHOV. "CONTINUUM SPECTROSCOPY OF HALO NUCLEI." International Journal of Modern Physics E 16, no. 04 (2007): 1033–45. http://dx.doi.org/10.1142/s0218301307006484.

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Halo nuclei represent a new type of structure found in extremely neutron rich light nuclei, at the limits of nuclear existence. Of particular interest are Borromean nuclei, where none of the binary substructures can bind. Similar structures, Efimov states, have now also been produced in traps in molecular physics. Nuclear physics has in recent years taken further steps to also explore the nature of the halo continuum, in fact the major part of the spectrum since halo nuclei support only one or a few bound states. Since 3 → 3 scattering is prohibitively difficult to perform, the halo continuum

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8

Kalmykov, N. N., V. N. Kalmykov, G. V. Kulikov, P. V. Sulakov, and Yu A. Fomin. "The light nuclei energy spectrum of primary cosmic rays using EAS MSU array data." Moscow University Physics Bulletin 63, no. 6 (2008): 425–27. http://dx.doi.org/10.3103/s0027134908060143.

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9

Wills, Beverley J., D. Wills, N. J. Evans, et al. "Polarization of IRAS Quasars and the Inner Structure of Active Galactic Nuclei." Symposium - International Astronomical Union 134 (1989): 325–26. http://dx.doi.org/10.1017/s0074180900141221.

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We have found that 4 new, bright IRAS quasars, out of 7 observed, have strong, non-variable, wavelength-dependent polarization. Three show degrees of polarization, pλ, increasing from infrared to UV wavelengths (Fig. 1), which implies a combination of a polarized, scattered spectrum and a much redder, unpolarized spectrum. Detailed IR and optical polarimetry and spectrophotometry of one, IRAS 13349+2438 (Wills et al.), shows a polarized flux spectrum, pλxFλ, (continuum and Pa α, Hα, and Hβ broad hydrogen lines) typical of unreddened, luminous quasars. This suggests that the path of scattered l

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10

BELYAEVA, T. L., and N. S. ZELENSKAYA. "Computation of Nuclear Reactions with Light-Heavy Ions." International Journal of Modern Physics C 02, no. 01 (1991): 238–42. http://dx.doi.org/10.1142/s012918319100024x.

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Анотація:

The computer code OLYMPS for calculation of the inclusive cross sections for nuclear reactions induced by light heavy ions on medium-mass nuclei at beam energies of 10–20 MeV per nucleon is developed. Our calculations are based on the description of the massive transfer reactions in the spectator model. In view of the fact that most of the considered reactions have more than two particles in the final state and require an allowance for the continuum spectrum, the standard distorted wave Born approximation (DWBA) code fails to work. In our method the transition amplitude is witten in a prior-fo

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