The flavor asymmetry in the polarized proton sea

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8513

Full metadata record

DC Field	Value	Language
dc.creator	Steffens F. M.	-
dc.date	2004	-
dc.date.accessioned	2013-06-01T11:22:45Z	-
dc.date.available	2013-06-01T11:22:45Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000200017	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2004&volume=34&issue=1a&spage=233	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/8513	-
dc.description	We perform a careful study on the effect of the Pauli blocking to the light polarized antiquark structure of the proton sea. We develop the formal expressions for the polarized antiquark distributions, highlighting the role played by quark statistics and the vacuum structure. The ratio involving the polarized antiquarks is calculated. In particular, it is found that D<img id="_x0000_i1026" src="../../../../img/revistas/bjp/v34n1a/a17img01.gif" align=absbottom>(x)/D<img id="_x0000_i1027" src="../../../../img/revistas/bjp/v34n1a/a17img02.gif" align=absbottom>(x) should be negative and x independent.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	The flavor asymmetry in the polarized proton sea	-
Appears in Collections:	Physics and Astronomy

Files in This Item:

There are no files associated with this item.

DSpace JSPUI