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Residues of higher order and holomorphic vector fields
Authors:Daniel Lehmann
Institution:(1) GETODIM, CNRS, UA 1407, Université de Montpellier II, Case 051 Place E. Bataillon, 34095 Montpellier cedex, France
Abstract:LetX 1 andX 2 be two holomorphic vector fields on a manifoldV with complex dimensionp. Assume that they have the same singular set sum. For all 
$$C_I  = (c_1 )^{i_1 }  \cdot (c_2 )^{i_2 }  \cdot  \cdot  \cdot (c_p )^{i_p } ,(i_1  + 2i_2  +  \cdot  \cdot  \cdot  + pi_p  = p)$$
, it is known (after Chern-Bott) that each of the vector fields defines a ldquoresidualrdquo characteristic classC 1(V,X 1)(resp.C 1(V,X 2)) inH 2p (V, V-sum), which is a lift of the usual characteristic classC 1 (V) of the tangent bundle. The differenceC 1 (V,X 2)-C 1 (V,X 1) belongs then to the image of part in the exact sequenceMediaObjects/10455_2005_BF02108292_f1.jpg. In fact, there exists a canonical liftC 1 (V,X 1,X 2) of this difference inH 2p–1(V-sum): we will call itthe residual class of order 2 (associated toI, X 1 andX 2). This class is localized near the points whereX 1 andX 2 are colinear: we will explain this precisely in terms of Grothendieck residues. The formula that we obtain can be interpreted as a generalization of the purely algebraic identity, obtained from the general one as a byproduct:MediaObjects/10455_2005_BF02108292_f2.jpg where (agr 1, ctdot, agrp) and (beta 1,ctdot, beta p ) denote two families of non-zero complex numbers, such that all denominators in this formula do not vanish. (This identity corresponds in fact to the case whereX 1 andX 2 are non-degenerate at the same isolated singular point.)If theagr i 's (1leilep) depend now differentiably (resp. holomorphically) on a real (resp. complex) parametert then, denoting by the derivative with respect tot, and assuming all numbers lying in a denominator not to be 0, we can deduce from the above identity the following derivation formula:MediaObjects/10455_2005_BF02108292_f3.jpg
Keywords:Holomorphic vector fields  Grothendieck residues  higher order
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