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1 nergies greater than approximately 6 MeV per nucleon.
2 the isotopic species with the same number of nucleons.
3 t to a mean field generated by all the other nucleons.
4 yproducts of their occasional recoil against nucleons.
5 10 x 10(6) to 40 x 10(6) electron volts per nucleon and an increasing galactic cosmic-ray electron i
6 energy spread and energies up to 18 MeV per nucleon and approximately 5% conversion efficiency (that
8 th at half-maximum approximately 0.5 MeV per nucleon) and a longitudinal emittance of less than 2 x 1
9 heavy ion (56)Fe radiation (energy: 1000 MeV/nucleon) and results were compared to gamma radiation do
13 ergy can be released by the rearrangement of nucleons between the initial- and final-state nuclei.
14 The ions have a mean energy of 3 MeV per nucleon (full-width at half-maximum approximately 0.5 Me
20 gment group by 137Cs gamma or Fe26+ (1.1 GeV/nucleon) irradiation vs the corresponding unirradiated D
28 c rays down to ~3 x 10(6) electron volts per nucleon, revealing H and He energy spectra with broad pe
30 ions (approximately62 megaelectron volts per nucleon) that peaked at approximately1.5RJ inside the br
33 ate the dynamics of quarks and gluons inside nucleons using deeply virtual Compton scattering (DVCS)-
34 ed to high energies (up to about 300 TeV per nucleon, where 1 TeV is 10(12) eV) in the expanding shoc
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