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THE LIFETIME OF A DEEPLY BOUND H DIBARYON AND THE CYGNUS-X-3 EVENTS
PHYSICS LETTERS B
  • JF Donoghue, University of Massachusetts Amherst
  • Eugene Golowich, University of Massachusetts - Amherst
  • BR Holstein, University of Massachusetts Amherst
Publication Date
1986
Abstract
The explanation of the Cygnus X-3 events which involves a strange-quark star emitting the doubly strange H dibaryon requires the H to have a lifetime of greater than ten years. We calculate the ΔS=2 H→ NN for an H bound below ΛN threshold, and find τHless, approximate6 days.
Disciplines
Comments
Published version is located at http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6TVN-46YSTRG-272&_user=1516330&_coverDate=07%2F17%2F1986&_alid=1524436710&_rdoc=1&_fmt=high&_orig=search&_origin=search&_zone=rslt_list_item&_cdi=5539&_sort=r&_st=13&_docanchor=&view=c&_ct=1&_acct=C000053443&_version=1&_urlVersion=0&_userid=1516330&md5=3572c42935734337556c605ab96fd8ea&searchtype=a
Pages
441-444
Citation Information
JF Donoghue, Eugene Golowich and BR Holstein. "THE LIFETIME OF A DEEPLY BOUND H DIBARYON AND THE CYGNUS-X-3 EVENTS" PHYSICS LETTERS B Vol. 174 Iss. 4 (1986)
Available at: http://works.bepress.com/barry_holstein/202/