scholarly journals Using a Spreadsheet To Solve the Schrödinger Equations for the Energies of the Ground Electronic State and the Two Lowest Excited States of H2

2014 ◽  
Vol 91 (6) ◽  
pp. 853-859 ◽  
Author(s):  
Yingbin Ge ◽  
Robert C. Rittenhouse ◽  
Jacob C. Buchanan ◽  
Benjamin Livingston
Keyword(s):  
Electronic State ◽  
Excited States ◽  
Ground Electronic State ◽  
Schrodinger Equations ◽  
Schrödinger Equations

Excited States of Li2 and the Ground Electronic State of Li 2 +

1985 ◽  
pp. 325-337
Author(s):  
R. A. Bernheim ◽  
L. P. Gold ◽  
C. A. Tomczyk
Keyword(s):  
Electronic State ◽  
Excited States ◽  
Ground Electronic State

scholarly journals Small solutions of nonlinear Schrödinger equations near first excited states

2012 ◽  
Vol 263 (3) ◽  
pp. 703-781 ◽  
Author(s):  
Kenji Nakanishi ◽  
Tuoc Van Phan ◽  
Tai-Peng Tsai
Keyword(s):  
Excited States ◽  
Nonlinear Schrödinger Equations ◽  
Schrodinger Equations ◽  
Schrödinger Equations ◽  
Nonlinear Schrödinger ◽  
Nonlinear Schrodinger Equations

scholarly journals The Populations of H2 Vibrational States in Intense UV Fields Near O-B Stars

1987 ◽  
Vol 115 ◽  
pp. 179-180
Author(s):  
P. E. Dewdney ◽  
R. S. Roger ◽  
N. Robert
Keyword(s):  
Electronic State ◽  
Excited States ◽  
Ground State ◽  
Molecular Hydrogen ◽  
Ground Electronic State ◽  
Vibrational States ◽  
Vibrationally Excited ◽  
B Stars ◽  
Intense Fields ◽  
The Mean

In most places where molecular hydrogen exists in the interstellar medium, it will be found in the ground vibrational and ground electronic state. This will not be so, however, near 0 or early B stars where, in the region just beyond the ionization boundary, populations will be determined by UV fields up to 105 times more intense than the mean interstellar value (4 × 10−16 ergs cm−3 s−1 = 1 Habing unit). The H2 absorbs Lyman-Werner band photons longwards of λ91 nm and subsequent decays to the ground electronic state may lead to dissociation (vibrational continuum) or to one of 14 vibrationally excited states. Molecules in these states have lifetimes of order 1010 s and, in the intense fields, will be exposed to further Lyman-Werner excitation. The probability of dissociation is therefore greatly enhanced by this ‘multiple excitation’, since the number of lines available to vibrationally excited H2 is many times that available to ground-state H2 (Shull, 1978).

New exact solutions of coupled (2+1)-dimensional nonlinear systems of Schrödinger equations

2011 ◽  
Vol 51 ◽  
pp. 110 ◽  
Author(s):  
F. Khani ◽  
M. T. Darvishi ◽  
Abbas Farmany ◽  
L. Kavitha
Keyword(s):  
Nonlinear Systems ◽  
Exact Solutions ◽  
Schrodinger Equations ◽  
Schrödinger Equations ◽  
New Exact Solutions
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