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                       Also, if the experiment was intended primarily to add to the body of published literature, it should be
                       acceptable to increase α to 0.05 or 0.10.
                        Having specified α, the investigator needs to specify β, or 1 − β. Cohen (1969) suggests that in the
                       context of medical treatments, a type I error is roughly four times as serious as a type II error. This
                       implies that one should use approximately β = 4α so that the power of the test is 1 − β  = 1 − 4α. Thus,
                       when α = 0.05, set 1 − β  = 0.80, or perhaps less.



                       Sample Size for Assessing the Equivalence of Two Means

                       The previous sections dealt with selecting a sample size that is large enough to detect a difference between
                       two processes. In some cases we wish to establish that two processes are not different, or at least are close
                       enough to be considered equivalent. Showing a difference and showing equivalence are not the same
                       problem.
                        One statistical definition of equivalence is the classical null hypothesis H 0 : η 1  − η 2  = 0 versus the
                       alternate hypothesis H 1 : η 1  − η 2  ≠ 0. If we use this problem formulation to determine the sample size for
                       a two-sided test of no difference, as shown in the previous section, the answer is likely to be a sample
                       size that is impracticably large when ∆ is very small.
                        Stein and Dogansky (1999) present an alternate formulation of this classical problem that is often
                       used in bioequivalence studies. Here the hypothesis is formed to demonstrate a difference rather than
                       equivalence. This is sometimes called the interval testing approach. The interval hypothesis (H 1 ) requires
                       the difference between two means to lie with an equivalence interval [θ L , θ U ] so that the rejection of
                       the null hypothesis, H 0  at a nominal level of significance (α), is a declaration of equivalence. The interval
                       determines how close we require the two means to be to declare them equivalent as a practical matter:


                                                                       –
                                              H 0 : η 1 η 2 ≤–  θ L  or  η 1 η 2 ≥  θ U
                       versus

                                                      H 1 : θ L <  η 1 η 2 <  θ U
                                                               –
                       This is decomposed into two one-sided hypotheses:


                                                                         –
                                            H 01 : η 1 η 2 ≤–  θ L  and  H 02 : η 1 η 2 ≥  θ U
                                                                         –
                                            H 11 : η 1 η 2 >–  θ L  H 12 : η 1 η 2 <  θ U
                       where each test is conducted at a nominal level of significance, α. If H 01  and H 02  are both rejected, we
                       conclude that   θ L <  η 1 η 2 <  θ U   and declare that the two treatments are equivalent.
                                        –
                                                                                                    2
                        We can specify the equivalence interval such that θ  = θ U  = −θ L . When the common variance σ  is
                       known, the rule is to reject H 0  in favor of H 1  if:
                                                – θ +  z α σ y 1 −y 2 ≤ y 1 − y 2 ≤  θ –  z α σ y 1 −y 2


                       The approximate sample size for the case where n 1  = n 2  = n is:
                                                          2σ z α +(  z β ) 2
                                                            2
                                                      n =  ------------------------------- +  1
                                                           ( θ ∆)  2
                                                              –
                       θ defines (a priori) the practical equivalence limits, or how close the true treatment means are required
                       to be before they are declared equivalent. ∆ is the true difference between the two treatment means under
                       which the comparison is made.
                       © 2002 By CRC Press LLC
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