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1 nergies greater than approximately 6 MeV per nucleon.
2 nd a solid-state mass containing unpolarized nucleons.
3 the isotopic species with the same number of nucleons.
4 t to a mean field generated by all the other nucleons.
5 yproducts of their occasional recoil against nucleons.
6 properties are governed by a single unpaired nucleon(1,2).
7 is encoded in the vector form factors of the nucleon(2).
8 ds to a single integral equation for the two-nucleon (2N) spin-singlet state, and four coupled integr
9     First, as previously, we show that for E/nucleon about 0.3 eV/nucleon water and nonwater containi
10  10 x 10(6) to 40 x 10(6) electron volts per nucleon and an increasing galactic cosmic-ray electron i
11  energy spread and energies up to 18 MeV per nucleon and approximately 5% conversion efficiency (that
12  volts (keV) to >/=50 megaelectron volts per nucleon and of electrons from >26 keV to >/=350 keV.
13 limits on coupling constants for the neutron-nucleon and proton-nucleon interactions in the range of
14 y the exotic interaction between unpolarized nucleons and polarized electrons.
15 th at half-maximum approximately 0.5 MeV per nucleon) and a longitudinal emittance of less than 2 x 1
16 heavy ion (56)Fe radiation (energy: 1000 MeV/nucleon) and results were compared to gamma radiation do
17 anced dose deposition provided by antiproton-nucleon annihilation.
18                   When protons and neutrons (nucleons) are bound into atomic nuclei, they are close e
19 esponding to closed shells of strongly bound nucleons) are particularly stable.
20               The QED calculation treats the nucleons as point-like, whereas the latter approach incl
21 ) from free proton targets and measuring the nucleon axial charge radius, r(A), to be 0.73 +/- 0.17 f
22 g-water target was irradiated with a 150 MeV/nucleon beam of (78)Kr at the National Superconducting C
23 ergy can be released by the rearrangement of nucleons between the initial- and final-state nuclei.
24 We set an experimental limit on the electron-nucleon coupling [Formula: see text] at the mediator bos
25 xial-vector electron coupling and the vector nucleon coupling for polarized electrons.
26 ramework that enables the inference of three-nucleon couplings in dense matter directly from astrophy
27 ers can offer stringent constraints on three-nucleon couplings, potentially at a level comparable to
28                         At sufficiently high nucleon densities, however, proton- and neutron-scatteri
29 tometer and a tungsten ring featuring a high nucleon density.
30  which are well constrained at typical inter-nucleon distances(1-5) but not at shorter distances.
31 reases in ion yield at equivalent energy per nucleon (E/m) values.
32 s between polarized neutrons and unpolarized nucleons for the force range of 0.03 to 100 meters, impr
33                                        Three-nucleon forces are suggested to drive Mo isotope structu
34 portion of the deuterons (i.e., above 10 MeV/nucleon) from the laser axis, a documented feature of th
35     The ions have a mean energy of 3 MeV per nucleon (full-width at half-maximum approximately 0.5 Me
36 interactions lead to hard collisions between nucleons, generating pairs of highly energetic nucleons
37 driven ions with energies of several MeV per nucleon have also been produced.
38       Understanding the interactions between nucleons in dense matter is an important challenge in th
39 emblance to the dynamical mass generation of nucleons in high-energy physics.
40 F(A)(Q(2)) has been extracted from the bound nucleons in neutrino-deuterium scattering(3-9), which re
41 including treatment of thermal scattering of nucleons in the continuum.
42                   Values of m, the number of nucleons in the revolving cluster, and of R, the radius
43 ns, we propose that the collective motion of nucleons in the ruptured neck of the fissioning system g
44 ectrons and the spin-polarized electrons and nucleons in three laboratory experiments.
45         As the relative momentum between two nucleons increases and their separation thereby decrease
46 eract with the nuclei of matter, the neutron-nucleon interaction provides unique information on light
47 straints for the couplings that govern three-nucleon interactions in chiral effective field theory.
48 constants for the neutron-nucleon and proton-nucleon interactions in the range of >=0.1 m (mediator b
49 c (> approximately 10 kiloelectron volts per nucleon) ion at closest approach.
50 gment group by 137Cs gamma or Fe26+ (1.1 GeV/nucleon) irradiation vs the corresponding unirradiated D
51 lei using a technique involving one- and two-nucleon knockout from beams of exotic nuclei.
52                                          Two-nucleon knockout or 'triple coincidence' reactions have
53 ay 7 post exposure to 0.5 Gy Fe ion (600 MeV/nucleon, Linear Energy Transfer (LET) = 175 keV/mum).
54                                The number of nucleons m in each cluster is taken to be 2 for neutron
55 ances and also support the use of point-like nucleon models with two- and three-body effective intera
56 ond, for water cluster beams at a constant E/nucleon, "molecular" ion yield increases with beam energ
57  measured from neutrino scattering from free nucleons, nu(mu)n -> mu(-)p and [Formula: see text], as
58 ts that around particular 'magic' numbers of nucleons, nuclear properties are governed by a single un
59          The matrix elements of relativistic nucleon-nucleon (NN) potentials are calculated directly
60 understanding of the short-range part of the nucleon-nucleon interaction.
61  from the strong, short-distance part of the nucleon-nucleon interaction.
62                                Values of the nucleon number of the revolving cluster are assigned on
63                                Values of the nucleon numbers of clusters and spheres, of the radius o
64 nergies ~195 to ~500 mega-electron volts per nucleon, of which we identify 15 (60)Fe nuclei.
65 en-dominated due to a local source of 50 MeV/nucleon oxygen.
66 s at a center-of-mass energy of 11.9 GeV per nucleon pair.
67 lectron scattering measurements that isolate nucleon pairs in short-distance, high-momentum configura
68 ns in a nucleus can form strongly correlated nucleon pairs.
69     Scattering of high energy particles from nucleons probes their structure, as was done in the expe
70  method to solve the quantum mechanical five-nucleon problem, we accurately determine the enhanced fu
71 roton from the SRC and detecting its partner nucleon (proton or neutron).
72       The strong nuclear interaction between nucleons (protons and neutrons) is the effective force t
73                    The internal structure of nucleons (protons and neutrons) remains one of the great
74  vector and axial vector form factors of the nucleon, providing an additional, complementary probe of
75 onstraints on axial-vector couplings between nucleons reach into a hitherto unexplored parameter spac
76 cleons, generating pairs of highly energetic nucleons referred to as short-range correlations (SRCs).
77 c rays down to ~3 x 10(6) electron volts per nucleon, revealing H and He energy spectra with broad pe
78  and four coupled integral equations for two-nucleon spin-triplet states, which are solved by an iter
79 s the latter approach includes the effect of nucleon structure in a systematic way.
80 ements in our capabilities to understand the nucleon structure in the weak sector, and also help the
81 e can provide the identity of a complex many-nucleon system(6,7).
82 ions (approximately62 megaelectron volts per nucleon) that peaked at approximately1.5RJ inside the br
83 tween quarks and gluons (the constituents of nucleons) that are described by the equations of quantum
84  more precise, providing a benchmark for few-nucleon theories, lattice quantum chromodynamics and ele
85 nique that involves the transfer of a single nucleon to the nucleus.
86 rely restricted the consistent range for the nucleon-to-photon ratio: 3.7 </= eta10 </= 4.0.
87                                          The nucleon transition axial form factor, F(A), can be measu
88 ate the dynamics of quarks and gluons inside nucleons using deeply virtual Compton scattering (DVCS)-
89 sly, we show that for E/nucleon about 0.3 eV/nucleon water and nonwater containing cluster beams gene
90 ed to high energies (up to about 300 TeV per nucleon, where 1 TeV is 10(12) eV) in the expanding shoc
91 al grains varies from about 2 to about 4 keV/nucleon, which falls within the range of the CSPN winds.
92 ed the acceleration of gold ions up to 7 MeV/nucleon with a strong dependency of the charge-state dis