Energy levels of atomic hydrogen

1985 ◽  
Vol 53 (11) ◽  
pp. 1038-1038
Author(s):  
T. C. Ernest Ma
2016 ◽  
Vol 714 ◽  
pp. 012009
Author(s):  
R Kh Gainutdinov ◽  
M A Khamadeev ◽  
O V Steryakov ◽  
K A Ziyatdinova ◽  
M Kh Salakhov

1996 ◽  
Vol 29 (8) ◽  
pp. 1573-1573 ◽  
Author(s):  
K Pachucki ◽  
D Leibfried ◽  
M Weitz ◽  
A Huber ◽  
W König ◽  
...  

2019 ◽  
pp. 259-322
Author(s):  
P.J.E. Peebles

This chapter examines applications drawn from perturbation theory. The main topic in perturbation theory is the energy and spontaneous decay rate of the 21-cm hyperfine line in atomic hydrogen. Before there were electronic computers, people had quite an accurate theoretical understanding of the energy levels in helium and more complicated systems. The trick was (and is) to find approximation schemes that treat unimportant parts of a physical system in quite crude approximations while reducing the interesting parts to a problem simple enough that it is feasible to compute but yet detailed enough to yield accurate results. The approximation methods in the chapter deal with the effects of small changes in the Hamiltonian, resulting for example from the application of a static or time variable electric or magnetic field. This may cause small changes in energy levels, and it may induce transitions among eigenstates of the original Hamiltonian.


2003 ◽  
Vol 49 ◽  
pp. 179-195
Author(s):  
Boris P. Stoicheff

Gerhard Herzberg, Nobel Laureate in Chemistry, had broad interests and achieved supreme accomplishments in physics, chemistry and astrophysics. The high points in his research were many. In physics they were the work on atomic hydrogen and helium, and evaluations of energy levels and constants of molecular hydrogen and its isotopes. His determinations of many molecular structures and discoveries of spectra of the free radicals CH 2 and CH 3 , and of the Rydberg molecule H3, were each outstanding contributions in chemistry. In astrophysics, his reproduction in the laboratory of the spectrum of CH + , proving its presence in the interstellar medium, and of spectra of C 3 and H 2 O + and their presence in comets, his observation of the quadrupole spectrum of H 2 and his discovery of hydrogen in the atmospheres of the planets opened up new applications of spectroscopy for our knowledge of the universe. His classic volumes on molecular spectra and molecular structures remain as encyclopaedias of molecular knowledge for all time. And his famous laboratory, the ‘Temple of spectroscopy’, served as a home for hundreds of scientists around the world, and helped to bring Canadian science to international prominence.


1996 ◽  
Vol 29 (2) ◽  
pp. 177-195 ◽  
Author(s):  
K Pachucki ◽  
D Leibfried ◽  
M Weitz ◽  
A Huber ◽  
W König ◽  
...  

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