Hamiltonian form of the Kemmer equation

dc.contributor.author	Zeleny, W.B.
dc.date.accessioned	2016-01-07T22:47:27Z
dc.date.available	2016-01-07T22:47:27Z
dc.date.issued	1967-06-25
dc.identifier.citation	Physical Review, Second Series, V. 158, no. 5, June 25, 1967, pp.1223-1225	en_US
dc.identifier.uri	https://hdl.handle.net/10945/47487
dc.description.abstract	The Hamiltonian form of the relativistic wave equation for bosons of spin 0 or 1 was first given by Kemmer. The problems associated with the redundant components of the wave function were later resolved by Heitler, who eliminated the redundant components by means of projection operators. We present an alternative treatment which yields essentially the same results as obtained by Heitler, but which retains all components of the wave function.	en_US
dc.format.extent	3 p.	en_US
dc.publisher	American Physical Society	en_US
dc.rights	This publication is a work of the U.S. Government as defined in Title 17, United States Code, Section 101. Copyright protection is not available for this work in the United States.	en_US
dc.title	Hamiltonian form of the Kemmer equation	en_US
dc.type	Article	en_US
dc.contributor.corporate	Naval Postgraduate School (U.S.)	en_US
dc.contributor.department	Physics	en_US
dc.description.distributionstatement	Approved for public release; distribution is unlimited.

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