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Page Title: Fast Fission Factor
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Infinite  Multiplication  Factor,  k
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Nuclear Physics and Reactor Theory Volume 2 of 2
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Reactor Theory (Nuclear Parameters) DOE-HDBK-1019/2-93 NEUTRON LIFE CYCLE Fast  Fission  Factor,  ( ) The first process that the neutrons of one generation may undergo is fast fission.   Fast fission is  fission caused by neutrons  that are in the fast energy range.   Fast fission results in the net increase in the fast neutron population of the reactor core.   The cross section for fast fission in uranium-235  or  uranium-238  is  small;  therefore,  only  a  small  number  of  fast  neutrons  cause fission.   The fast neutron population in one generation is therefore increased by a factor called the fast fission factor.  The fast fission factor (  ) is defined as the ratio of the net number of fast neutrons produced by all fissions to the number of fast neutrons produced by thermal fissions. The mathematical expression of this ratio is shown below.                                                                                         number  of  fast  neutrons  produced  by  all  fissions number  of  fast  neutrons  produced  by  thermal  fissions In  order  for  a  neutron  to  be  absorbed  by  a  fuel  nucleus  as  a  fast  neutron, it  must  pass  close enough  to  a  fuel  nucleus  while  it  is  a  fast  neutron.    The  value  of      will  be  affected  by  the arrangement and concentrations of the fuel and the moderator.  The value of   is essentially 1.00 for a homogenous reactor where the fuel atoms are surrounded by moderator atoms.   However, in a heterogeneous  reactor, all the fuel atoms are packed closely together in elements such as pins,  rods,  or  pellets.    Neutrons  emitted  from  the  fission  of  one  fuel  atom  have  a  very  good chance of passing near another fuel atom before slowing down significantly.   The arrangement of the core elements results in a value of about 1.03 for   in most heterogeneous reactors.   The value of   is not significantly affected by variables such as temperature, pressure, enrichment, or neutron poison concentrations.  Poisons are non-fuel materials that easily absorb neutrons and will be discussed in more detail later. Resonance  Escape  Probability,  (p) After  increasing  in number  as  a  result of  some  fast  fissions, the  neutrons  continue  to diffuse through the reactor.  As the neutrons move they collide with nuclei of fuel and non-fuel material and  moderator  in  the  reactor  losing  part  of  their  energy  in  each  collision  and  slowing  down. While they are slowing down through the resonance region of uranium-238, which extends from about 6 eV to 200 eV, there is a chance that some neutrons will be captured.   The probability that  a  neutron  will  not  be  absorbed  by  a  resonance  peak  is  called  the  resonance  escape probability.    The  resonance  escape  probability  (p)  is  defined  as  the  ratio  of  the  number  of neutrons that reach thermal energies to the number of fast neutrons that start to slow down.  This ratio is shown below. p   number  of  neutrons  that  reach  thermal  energy number  of  fast  neutrons  that  start  to  slow  down Rev. 0 NP-03 Page 3

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