nips nips2004 nips2004-69 knowledge-graph by maker-knowledge-mining

69 nips-2004-Fast Rates to Bayes for Kernel Machines


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Author: Ingo Steinwart, Clint Scovel

Abstract: We establish learning rates to the Bayes risk for support vector machines (SVMs) with hinge loss. In particular, for SVMs with Gaussian RBF kernels we propose a geometric condition for distributions which can be used to determine approximation properties of these kernels. Finally, we compare our methods with a recent paper of G. Blanchard et al.. 1

Reference: text


Summary: the most important sentenses genereted by tfidf model

sentIndex sentText sentNum sentScore

1 gov Abstract We establish learning rates to the Bayes risk for support vector machines (SVMs) with hinge loss. [sent-2, score-0.408]

2 In particular, for SVMs with Gaussian RBF kernels we propose a geometric condition for distributions which can be used to determine approximation properties of these kernels. [sent-3, score-0.369]

3 Since by the no-free-lunch theorem of Devroye (see [4]) performance guarantees are impossible without assumptions on the data-generating distribution we will restrict our considerations to specific classes of distributions. [sent-13, score-0.216]

4 In particular, we will present a geometric condition which describes how distributions behave close to the decision boundary. [sent-14, score-0.391]

5 This condition is then used to establish learning rates for SVM’s. [sent-15, score-0.328]

6 To obtain learning rates faster than n−1/2 we also employ a noise condition of Tsybakov (see [5]). [sent-16, score-0.415]

7 Combining both concepts we are in particular able to describe distributions such that SVM’s with Gaussian kernel learn almost linearly, i. [sent-17, score-0.184]

8 To make this precise the risk of a measurable function f : X → R is defined by RP (f ) := P {(x, y) : sign f (x) = y} . [sent-34, score-0.138]

9 The smallest achievable risk RP := inf RP (f ) | f : X → R measurable is called the Bayes risk of P . [sent-35, score-0.239]

10 A function fP : X → Y attaining this risk is called a Bayes decision function. [sent-36, score-0.167]

11 The next naturally arising question is whether there are classifiers which guarantee a specific rate of convergence in (1) for all distributions. [sent-39, score-0.148]

12 However, if one restricts considerations to certain smaller classes of distributions such rates exist for various classifiers, e. [sent-43, score-0.335]

13 : • Assuming that the conditional probability η(x) := P (1|x) satisfies certain smoothness assumptions Yang showed in [6] that some plug-in rules (cf. [sent-45, score-0.19]

14 [4]) achieve rates for (1) which are of the form n−α for some 0 < α < 1/2 depending on the assumed smoothness. [sent-46, score-0.188]

15 He also showed that these rates are optimal in the sense that no classifier can obtain faster rates under the proposed smoothness assumptions. [sent-47, score-0.499]

16 1]) that using structural risk minimization over a sequence of hypothesis classes with finite VC-dimension every distribution which has a Bayes decision function in one of the hypothesis classes can be learned with rate n−1/2 . [sent-50, score-0.416]

17 If F contains a Bayes decision function then up to a logarithmic factor the convergence rate of the ERM classifier over F is n−1 (see [4, Sec. [sent-54, score-0.183]

18 Restricting the class of distributions for classification always raises the question of whether it is likely that these restrictions are met in real world problems. [sent-57, score-0.136]

19 We conclude that the above listed rates are established for situations which are rarely met in practice. [sent-62, score-0.302]

20 Considering the ERM classifier and hypothesis classes F containing a Bayes decision function there is a large gap in the rates for noise-free and noisy distributions. [sent-63, score-0.383]

21 In [5] Tsybakov proposed a condition on the noise which describes intermediate situations. [sent-64, score-0.233]

22 In order to present this condition we write η(x) := P (y = 1|x), x ∈ X, for the conditional probability and PX for the marginal distribution of P on X. [sent-65, score-0.131]

23 We will use the following modified version of Tsybakov’s noise condition which describes the size of the latter regions: Definition 1. [sent-68, score-0.233]

24 We say that P has Tsybakov noise exponent q if there exists a constant C > 0 such that for all sufficiently small t > 0 we have PX |2η − 1| ≤ t ≤ C · tq . [sent-70, score-0.763]

25 (2) All distributions have at least noise exponent 0. [sent-71, score-0.803]

26 In particular this means that noise-free 2 distributions have exponent q = ∞. [sent-73, score-0.714]

27 Finally note, that Tsybakov’s original noise condition q assumed PX (f = fP ) ≤ c(RP (f ) − RP ) 1+q for all f : X → Y which is satisfied if e. [sent-74, score-0.224]

28 In [5] Tsybakov showed that if P has a noise exponent q then ERM-type classifiers can q+1 obtain rates in (1) which are of the form n− q+pq+2 , where 0 < p < 1 measures the complexity of the hypothesis class. [sent-78, score-1.098]

29 In particular, rates faster than n−1/2 are possible whenever q > 0 and p < 1. [sent-79, score-0.22]

30 Furthermore, his classifier requires substantial knowledge on how to approximate the Bayes decision rules of the considered distributions. [sent-81, score-0.139]

31 2 Results In this paper we will use the Tsybakov noise exponent to establish rates for SVM’s which are very similar to the above rates of Tsybakov. [sent-83, score-1.173]

32 To this end let H be a reproducing kernel Hilbert space (RKHS) of a kernel k : X × X → R, i. [sent-85, score-0.194]

33 Now given a regularization parameter λ > 0 the decision function of an SVM is n 1 2 (fT,λ , bT,λ ) := arg min λ f H + l yi (f (xi ) + b) , (3) f ∈H n i=1 b∈R where l(t) := max{0, 1 − t} is the so-called hinge loss. [sent-94, score-0.164]

34 Unfortunately, only a few results on learning rates for SVM’s are known: In [8] it was shown that SVM’s can learn with linear rate if the distribution is noise-free and the two classes can be strictly separated by the RKHS. [sent-95, score-0.325]

35 For RKHS which are dense in the space C(X) of continuous functions the latter condition is satisfied if the two classes have strictly positive distance in the input space. [sent-96, score-0.211]

36 Furthermore, Wu and Zhou (see [9]) recently established rates under the assumption that η is contained in a Sobolev space. [sent-98, score-0.244]

37 In particular, they proved rates of the form (log n) −p for some p > 0 if the SVM uses a Gaussian kernel. [sent-99, score-0.188]

38 Obviously, these rates are much too slow to be of practical interest and the difficulties with smoothness assumptions have already been discussed above. [sent-100, score-0.288]

39 Furthermore, we define the approximation error function by a(λ) := inf λ f f ∈H 2 H + Rl,P (f ) − Rl,P , λ ≥ 0. [sent-105, score-0.129]

40 However, in non-trivial situations no rate of convergence which uniformly holds for all distributions P is possible. [sent-109, score-0.191]

41 Then H approximates P with exponent β ∈ (0, 1] if there is a C > 0 such that for all λ > 0: a(λ) ≤ Cλβ . [sent-112, score-0.697]

42 Because of the specific structure of the approximation error function values β > 1 are only possible for distributions with η ≡ 1 . [sent-114, score-0.129]

43 Then H has complexity exponent 0 < p ≤ 2 if there is an ap > 0 such that for all ε > 0 we have log N (BH , ε, C(X)) ≤ ap ε−p . [sent-123, score-0.798]

44 Note, that in [10] the complexity exponent was defined in terms of N (BH , ε, L2 (TX )), where L2 (TX ) is the L2 -space with respect to the empirical measure of (x1 , . [sent-124, score-0.733]

45 3 Let H be a RKHS of a continuous kernel on X with complexity exponent 0 < p < 2, and let P be a probability measure on X × Y with Tsybakov noise exponent 0 < q ≤ ∞. [sent-140, score-1.624]

46 Furthermore, assume that H approximates P with exponent 0 < β ≤ 1. [sent-141, score-0.697]

47 3 these rates have the form n− (2q+pq+4)(1+β) +ε for all ε > 0. [sent-149, score-0.188]

48 5 For brevity’s sake our major aim was to show the best possible rates using our techniques. [sent-151, score-0.188]

49 3 states rates for the SVM under the assumption that (λn ) is optimally chosen. [sent-153, score-0.188]

50 However, we emphasize, that the techniques of [10] also give rates if (λn ) is chosen in a different (and thus sub-optimal) way. [sent-154, score-0.188]

51 If we rescale the complexity exponent p from (0, 2) to (0, 1) and write p for the new complexity − q+1 exponent this rate becomes n q+p q+2 . [sent-162, score-1.491]

52 It also suffices to suppose that H approximates P with exponent β for all β < β, and that H has complexity exponent p for all p > p. [sent-168, score-1.401]

53 Now, it is shown in [10] that the RKHS H has an approximation exponent β = 1 if and only if H contains a minimizer of the l-risk. [sent-169, score-0.728]

54 In particular, if H has approximation exponent β for all β < 1 but not for β = 1 then H does not contain such a minimizer but Theorem 2. [sent-170, score-0.728]

55 If in addition the RKHS consists of C ∞ functions we can choose p arbitrarily close to 0, and hence we can obtain rates up to n−1 even though H does not contain a minimizer of the l-risk, that means e. [sent-172, score-0.231]

56 In particular this seems to be true for the most popular kernel, that is the Gaussian RBF kernel kσ (x, x ) = exp(−σ 2 x − x 2 ), 2 x, x ∈ X on (compact) subsets X of Rd with width 1/σ. [sent-177, score-0.131]

57 However, to our best knowledge no non-trivial condition on η or fP = sign ◦(2η − 1) which ensures an approximation exponent β > 0 for fixed width has been established and [12] shows that Gaussian kernels poorly approximate smooth functions. [sent-178, score-0.946]

58 Hence plug-in rules based on Gaussian kernels may perform poorly under smoothness assumptions on η. [sent-179, score-0.192]

59 In particular, many types of SVM’s using other loss functions are plug-in rules and therefore, their approximation properties under smoothness assumptions on η may be poor if a Gaussian kernel is used. [sent-180, score-0.268]

60 However, our SVM’s are not plug-in rules since their decision functions approximate the Bayes decision function (see [13]). [sent-181, score-0.238]

61 Intuitively, we therefore only need a condition that measures the cost of approximating the “bump” of the Bayes decision function at the “decision boundary”. [sent-182, score-0.204]

62 We will now establish such a condition for Gaussian RBF kernels with varying widths 1/σ n . [sent-183, score-0.192]

63 Since we are only interested in distributions P having a Tsybakov exponent q > 0 we always assume that X = X −1 ∪ X1 holds PX -almost surely. [sent-186, score-0.729]

64 With the help of this function we can define the following geometric condition for distributions: Definition 2. [sent-190, score-0.188]

65 We say that P has geometric noise exponent α ∈ (0, ∞] if we have X −αd τx |2η(x) − 1|PX (dx) < ∞ . [sent-192, score-0.871]

66 (6) Furthermore, P has geometric noise exponent ∞ if (6) holds for all α > 0. [sent-193, score-0.886]

67 In the above definition we make neither any kind of smoothness assumption nor do we assume a condition on PX in terms of absolute continuity with respect to the Lebesgue measure. [sent-194, score-0.146]

68 Instead, the integral condition (6) describes the concentration of the measure |2η −1|dPX near the decision boundary. [sent-195, score-0.246]

69 The less the measure is concentrated in this region −1 the larger the geometric noise exponent can be chosen. [sent-196, score-0.874]

70 Using this interpretation we easily can construct distributions which have geometric noise exponent ∞ and touching classes. [sent-201, score-0.911]

71 9 We say that η is H¨ lder about 1 with exponent γ > 0 on X ⊂ Rd if there is o 2 a constant cγ > 0 such that for all x ∈ X we have γ (7) |2η(x) − 1| ≤ cγ τx . [sent-204, score-0.755]

72 If η is H¨ lder about 1/2 with exponent γ > 0, the graph of 2η(x) − 1 lies in a multiple o γ γ of the envelope defined by τx at the top and by −τx at the bottom. [sent-205, score-0.729]

73 To be H¨ lder about o 1/2 it is sufficient that η is H¨ lder continuous, but it is not necessary. [sent-206, score-0.214]

74 A function which is o H¨ lder about 1/2 can be very irregular away from the decision boundary but it cannot jump o ¨ across the decision boundary discontinuously. [sent-207, score-0.391]

75 In addition a Holder continuous function’s ¨ exponent must satisfy 0 < γ ≤ 1 where being Holder about 1/2 only requires γ > 0. [sent-208, score-0.673]

76 ¨ For distributions with Tsybakov exponent such that η is Holder about 1/2 we can bound the geometric noise exponent. [sent-209, score-0.911]

77 Indeed, let P be a distribution which has Tsybakov noise ¨ exponent q ≥ 0 and a conditional probability η which is Holder about 1/2 with exponent γ > 0. [sent-210, score-1.422]

78 Then (see [10]) P has geometric noise exponent α for all α < γ q+1 . [sent-211, score-0.845]

79 d For distributions having a non-trivial geometric noise exponent we can now bound the approximation error function for Gaussian RBF kernels: Theorem 2. [sent-212, score-0.974]

80 10 Let X be the closed unit ball of the Euclidian space Rd , and Hσ be the RKHS of the Gaussian RBF kernel kσ on X with width 1/σ > 0. [sent-213, score-0.179]

81 Furthermore, let P be a distribution with geometric noise exponent 0 < α < ∞. [sent-214, score-0.883]

82 Roughly α speaking this states that the family of spaces Hσ(λ) approximates P with exponent α+1 . [sent-221, score-0.727]

83 Note, that we can obtain approximation rates up to linear order in λ for sufficiently benign distributions. [sent-222, score-0.251]

84 The price for this good approximation property is, however, an increasing complexity of the hypothesis class Hσ(λ) for σ → ∞, i. [sent-223, score-0.186]

85 The following theorem estimates this in terms of the complexity exponent: Theorem 2. [sent-226, score-0.183]

86 T ∈Z n Having established both results for the approximation and complexity exponent we can now formulate our main result for SVM’s using Gaussian RBF kernels: Theorem 2. [sent-229, score-0.823]

87 12 Let X be the closed unit ball of the Euclidian space Rd , and P be a distribution on X × Y with Tsybakov noise exponent 0 < q ≤ ∞ and geometric noise exponent 0 < α < ∞. [sent-230, score-1.656]

88 3 Discussion of a modified support vector machine Let us now discuss a recent result (see [11]) on rates for the following modification of the original SVM: n 1 ∗ fT,λ := arg min λ f H + l yi f (xi ) . [sent-240, score-0.254]

89 To describe the result of [11] we need the following modification of the approximation error function: a∗ (λ) := inf λ f f ∈H H + Rl,P (f ) − Rl,P , λ ≥ 0. [sent-242, score-0.129]

90 1 Let H be a RKHS of a continuous kernel on X with complexity exponent 0 < p < 2, and let P be a distribution on X × Y with Tsybakov noise exponent ∞. [sent-248, score-1.595]

91 If H has complexity exponent p it can be shown that these eigenvalues decay at least as fast as n−2/p . [sent-253, score-0.704]

92 It was also mentioned in [11] that using the techniques therein it is possible to derive rates for the original SVM. [sent-257, score-0.217]

93 To this end let us suppose that H approximates P with exponent 0 < β ≤ 1, i. [sent-267, score-0.761]

94 Therefore, if H 4β approximates P with exponent β then the rate in Theorem 3. [sent-272, score-0.754]

95 It is naturally to ask whether a similar observation can be made if we have a Tsybakov noise exponent which is smaller than ∞. [sent-278, score-0.737]

96 Furthermore, the asymptotically optimal choice of λn is again independent of the approximation exponent β. [sent-282, score-0.685]

97 However, it depends on the (typically unknown) noise exponent q. [sent-283, score-0.737]

98 12 if P has a non-trivial geometric noise exponent α? [sent-287, score-0.845]

99 Consistency of support vector machines and other regularized kernel machines. [sent-301, score-0.129]

100 On the influence of the kernel on the consistency of support vector machines. [sent-331, score-0.131]


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[(13, 0.098), (15, 0.134), (26, 0.121), (31, 0.086), (33, 0.165), (35, 0.014), (39, 0.039), (44, 0.132), (50, 0.124)]

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