scholarly journals Influence of the Coulomb exchange term on nuclear single-proton resonances

2016 ◽  
Vol 27 (5) ◽  
Author(s):  
Shu-Yang Wang ◽  
Zhong-Lai Zhu ◽  
Zhong-Ming Niu
2014 ◽  
Vol 89 (3) ◽  
Author(s):  
Zhong-Lai Zhu ◽  
Zhong-Ming Niu ◽  
Dong-Peng Li ◽  
Quan Liu ◽  
Jian-You Guo

2008 ◽  
Vol 39 (01) ◽  
Author(s):  
U Gruber-Sedlmayr ◽  
M Brunner-Krainz ◽  
E Sorantin ◽  
W Sauseng ◽  
B Plecko

1994 ◽  
Vol 59 (11) ◽  
pp. 2523-2532 ◽  
Author(s):  
John Hondrelis ◽  
John Matsoukas ◽  
George Agelis ◽  
Paul Cordopatis ◽  
Ning Zhou ◽  
...  

The conformation of [Sar1]angiotensin II in water at neutral pH has been examined by proton magnetic resonance spectroscopy at 400 MHz and in particular by comparing its 1H NMR spectral data with those of analogues modified at positions 1,4 and 6, namely [Sar1,Cha8]ANGII, [Des Asp1,Cha8]ANGII, [Aib1,Tyr(Me)4]ANGII, [Aib1,Tyr(Me)4,Ile8]ANGII, [N-MeAib1,Tyr(Me)4]ANGII, [N-MeAib1,Tyr(Me)4,Ile8]ANGII, ANGIII and [Sar1,Ile8]ANGII. Assignment of all proton resonances in these analogues was made possible by 2D COSY NMR experiments. The H-2 and H-4 protons for the histidine ring in [Sar1]ANGII, ANGII and ANGIII were shielded compared with the same protons in [Sar1,Ile8]ANGII, [Sar1,Cha8]ANGII and [Des Asp1,Cha8]ANGII; this shielding effect was not disturbed upon methylation of the tyrosine hydroxyl and/or replacement of residue 1 (sarcosine or aspartic acid) with aminoisobutyric acid (Aib) or N-methyl aminoisobutyric acid (N-MeAib). These data are consistent with our previous suggestion based on NMR studies in neutral DMSO that a characteristic folded conformation for ANGII previously observed in non-polar solvents can also be detected in water at neutral pH, but to a lesser degree.


1983 ◽  
Vol 130 (3-4) ◽  
pp. 134-138 ◽  
Author(s):  
Ch. Stoyanov ◽  
A.I. Vdovin

2002 ◽  
Vol 352 (5-6) ◽  
pp. 415-420 ◽  
Author(s):  
Elena Falkovskaia ◽  
Vasyl G. Pivovarenko ◽  
Juan Carlos del Valle

1946 ◽  
Vol 70 (11-12) ◽  
pp. 891-893 ◽  
Author(s):  
L. I. Schiff
Keyword(s):  

2003 ◽  
Vol 21 (6) ◽  
pp. 1289-1294 ◽  
Author(s):  
H. J. Fahr

Abstract. Many hydrodynamic models have been presented which give similar views of the interaction of the solar wind plasma bubble with the counterstreaming partially ionized interstellar medium. In the more recent of these models it is taken into account that the solar and interstellar hydrodynamic flows of neutral atoms and protons are coupled by mass-, momentum-, and energy-exchange terms due to charge exchange processes. We shall reinvestigate the theoretical basis of this coupling here by use of a simplified description of the heliospheric interface and describe the main physics of the H-atom penetration through the more or less standing well-known plasma wall ahead of the heliopause. Thereby we can show that the type of charge exchange coupling terms used in up-to-now hydrodynamic treatments unavoidably leads to an O-type critical point at the sonic point of the H-atom flow, thus not allowing for a continuation of the integration of the hydrodynamic set of differential equations. The remedy for this problem is given by a more accurate formulation of the momentum exchange term for quasi-and sub-sonic H-atom flows. With a refined momentum exchange term derived from basic kinetic Boltzmann principles, we instead arrive at a characteristic equation with an X-type critical point, allowing for a continuous solution from supersonic to subsonic flow conditions. This necessitates that the often treated problem of the propagation of inter-stellar H-atoms through the heliosheath has to be solved using these newly derived, differently effective plasma – gas friction forces. Substantially different results are to be expected from this context for the filtration efficiency of the heliospheric interface.Key words. Interplanetary physics (heliopause and solar wind termination; interstellar gas) – Ionosphere (plasma temperature and density)


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