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12. Models of Recombination
                              260
                              where T ranges over all subsets of {1,... ,k} and |S ∩ T| indicates the
                              number of elements in the intersection S ∩ T. This last formula continues
                              to hold when the fixed counts n i are replaced by the random counts N I i
                              Taking expectations therefore produces
                                     y S  =E(y N S )                                          .
                                              1  k

                                         =           (−1) |S∩T |  Pr  N I i  =0           (12.6)
                                              2
                                                   T             i∈T
                                                   1      1                 k
                                              1  k      	         k

                                         =            ···   (−1)  i=1  s i t i  Pr  t i N I i  =0 ,
                                              2
                                                  t 1 =0  t k =0            i=1
                              where s i =1 {i∈S} and t i =1 {i∈T } are the obvious indicator functions.
                              This is the sought-after generalization of Mather’s formula [24, 26]. It col-
                              lectively expresses the multilocus gamete probabilities as the inverse Walsh
                              transform of the avoidance probabilities of the chiasma process.
                                Special cases of (12.6) are easy to construct. For instance, Mather’s for-
                                                                 1
                                                                 2
                              mula (12.1) can be restated as y {1} = [1 − Pr(N I 1  = 0)] for k = 1. The
                                                                  1
                                                                  2
                              probability of nonrecombination is y ∅ = [1 + Pr(N I 1  = 0)]. When k =2,
                              two of the relevant gamete probabilities are
                                         y {1}
                                         1
                                      =    [1 − Pr(N I 1  = 0)+Pr(N I 2  =0) − Pr(N I 1  + N I 2  =0)
                                         4
                                                                                          (12.7)
                                         y {1,2}
                                         1
                                      =    [1 − Pr(N I 1  =0) − Pr(N I 2  = 0)+Pr(N I 1  + N I 2  = 0)].
                                         4
                              12.3 Count-Location Model
                              The count-location model operates by first choosing the total number N of
                              chiasmata along the bundle of four chromatids [13, 23]. If we identify the
                              bundle with the unit interval [0, 1], then N = N [0,1] . Let q n =Pr(N = n)
                              be the distribution of N. Once the number of chiasmata is chosen, the
                              individual chiasmata are located independently along the bundle according
                              to some common continuous distribution F(t). If λ =E(N) in this setting,
                                                                                1
                              then the map length of an interval [a, b] reduces to d = λ[F(b) − F(a)].
                                                                                2
                              The recombination fraction θ of the interval can be expressed compactly
                                                                ∞     n
                              via the generating function Q(s)=  n=0 n s of N. Conditioning on the
                                                                   q
                              value of N, we find that
                                                   1
                                            θ  =    Pr(N [a,b] > 0)
                                                   2
                                                     ∞
                                                   1
                                               =        q n [1 − Pr(N [a,b] =0 | N = n)]
                                                   2
                                                    n=0
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