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The first in situ electron paramagnetic resonance (EPR) spectroelectrochemical study of C60 fullerene peapods (C60@SWCNT) as well as that of single-walled carbon nanotubes (SWCNTs) in different electrolyte solutions describes the formation of spin states by charge transfer reactions.
The corresponding spectral curve (endmember 1) in Fig. 11f has a characteristic bump at about ≈ − 100 meV and a vanishing density of states at around the Fermi level likely associated with a formation of spin density wave gap below T = 119 K [77].
Therefore, alternative methods to facilitate hEB formation and culture systems have been explored, including stirred suspension cultures [9], [10], bioreactor cultures [11], and the formation of spin EBs that are aggregated by centrifugation [12], [13].
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Besides licensing IPs to existing firms, TTOs may facilitate the formation of spin-offs by providing technology and business incubation services to their researchers.
The formation of spin-echoes in the Carr-Purcell-Meiboom Gill (CPMG) NMR experiment on rubbery polybutadiene (PBD) has been studied as a function of temperature and CPMG inter-pulse spacing.
The formation of spinning detonation thus not only depends on the high instability of detonation and channel dimension in the transverse directions, but also depends on the initial perturbation.
This technique is based on the nucleophilic addition of superoxide to a diamagnetic cyclic nitrone, referred to as the spin trap, and the formation of a spin adduct, i.e. a persistent radical with a characteristic EPR spectrum.
Key elements of the sequence are insensitivity to calibration of the transmit gain, the formation of a spin echo giving high-quality spectral information, and a small effective tip angle that preserves the magnetization for a sufficient duration.
In higher fields, however, the magnetization does not saturate and is still increasing at the limiting field of 5 T. The shape of the low T isothermal magnetization is consistent with the formation of a spin or cluster glass on cooling T < Tf.
The entire star is not taken in by the black hole, since much of the falling envelope of the star either rebounds from the temporary formation of a spinning neutron core or misses passing through the very centre of the core and is spun off instead.
This paper presents findings from an analysis of the determinants of the formation of university spin-off companies within the university's research park.
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