INVERSES OF PERTURBED LAPLACE-KIRCHHOFF AND SOME DISTANCE MATRICES

Milan Kunz

Jurkovičova 13, 63800 Brno, Czech Republic

ABSTRACT

It is shown that generalized inverse matrices of Laplace-Kirchhoff matrices, Eichinger matrices E, are inverse matrices of perturbed Laplace-Kirchhoff matrices. Similarly, singular distance matrices have inverses, when perturbed. The slightest perturbation is necessary for long chains.

Introduction

Properties of chemical bonds of molecules are related with eigenvalues of their adjacency matrices A, which were therefore studied intensively [1]. Great interest was paid to distance matrices D. They are connected with the oldest topological index, the Wiener number W, which is one half of the sum of elements of the distance matrix [2,3].

Only recently, chemical applications of Laplace-Kirchhoff matrices aroused interest [4-9], although they have been used in crystallography [10].

The Laplace-Kirchhoff matrix is a quadratic form of the incidence matrix S of an oriented graph

STS = V - A (1)

where V is the diagonal matrix of vertex degrees, and STis the transposed matrix S.

For linear chains and simple n-cycles Eichinger [11] defined generalized inverses to the corresponding Laplace-Kirchhoff matrices by way of the matrix equation

STSE = nU (2)where U is the generalized unit matrix :U = I - 1/n JJTI is the diagonal unit matrix,J is the unit vector-column,nU is identical with the Laplace-Kirchhoff matrix of the complete graph, n being the number of vertices.

Recently, Klein and Randic [12] proposed for finding the generalized inverses of STS equation (3)

Ω = (STS + JTJ) - cJT J (3)

where they used the constant c=1/n , and applied such inverses for finding the resistance distances in graphs.

I found that some classes (and examples of small graphs) of matrices obtained by a Moebius inversion of the Ulam sub-graph conjecture [13]

E = S (djSTS) (4)

where djM is the matrix M with jth row and column deleted (their elements are zeroes), have properties of the generalized inverse of the Laplace-Kirchhoff matrices.

The elements of such E matrices (E as Eichinger) of trees correspond to distance sums, ejj is the sum of distances of the vertex j to all other vertices Sjdij, eij for i š j is the sum of distances of the vertex i diminished by walks passed between vertices i and j. The inverses E were verified at trees, simple n-cycles and complete graphs by direct counts. For simple n-cycles, the elements of the Eichinger matrices are

 

 

and for complete graphs E = U.

The generalized inverses of STS according to the equations (3) and (4) differ sometimes. E. g. for star S4

 

Equation 3

Equation 4

1/16

3

-1

-1

-1

1/4

3

2

2

2

-1

11

-5

-5

2

5

1

1

-1

-5

11

-5

2

1

5

1

-1

- 5

-5

11

2

1

1

5

Since STSJTJ = 0, there can be infinite many generalized inverses of STS differing by

cJTJ.

Eichinger matrices with known elements have an important property. They are nonsingular and therefore they have inverses E-1 with the properties

STS = nUE-1EE-1 = I

In this paper inverses of Eichinger and distance matrices of several types of graphs are studied.

Perturbed Laplace-Kirchhoff matrices

The difference matrix X between a Laplace-Kirchhoff matrix STS and the inverse of its Eichinger matrix must yield the difference between matrices I and U, which is 1/nJJT.

(STS + X)E = U + 1/nJJT = I.

Because the row and column sums of Eichinger matrices are constant, it was possible to formulate the following conjecture and prove it for trees, simple cycles and complete graphs.

Conjecture: An Eichinger matrix is the inverse of the Laplace-Kirchhoff matrix perturbed by a fraction c of the quadratic unit matrix

E = S (djSTS)-1 = (STS + cJJT)-1

Proof for trees: The trace elements of Eichinger matrices E of trees are distances of the vertex j to all other vertices. Each distance dij is counted twice, thus Tr(E) = 2W, where W is the Wiener number. Other matrix elements in all rows and columns are distances unpassed during all walks between the given vertex i to all other vertices 1 till n. Their sum is just the distances passed between all vertices, again the Wiener number W. Therefore the corrective constant for trees is c = 1/W.

Proof for simple cycles: From the recurrence relation for Eichinger matrices of simple cycles [13] follows, that row and column sums of their elements are constant, too. They are given by the sums of binomial coefficients

 

Proof for complete graphs: It is given by the definition. The sum of matrix elements is just (n - 1) = 1/c.

Interesting results were obtained for a disconnected graph, e. g. G = L2 + L3. It was necessary to find at first the Eichinger matrix of its complement GC = (K - G) and its inverse. E-1(GC) is the corresponding Laplace-Kirchhoff matrix perturbed by noise elements in the range n = 0.0310 to 0.0313. The Eichinger matrix E(G) was then found as the difference E(G) = E(K) - E(GC). Its elements were rather large numbers. Nevertheless, the product STSE was a surprisingly simple matrix. It was the Laplace-Kirchhoff matrix of K2 + K3 with different multiplicities of both components.

The Laplace-Kirchhoff matrices of disconnected graphs have as many zero eigenvalues as the corresponding graphs have components. Even if all zero eigenvalues are removed by perturbation, they are restored by multiplication with their inverses.

Inverses of some distance matrices

Křivka and Trinajstic [14] determined distance topological polynomials of some classes of graphs. It follows, that topological distance matrices of even-membered cycles have no inverse, because their determinant det [D] is zero, but for certain classes of graphs, D-1 do exist. The elements of D-1 will be formulated in the form DD-1 = bI, to avoid complicated fractions.

(i) D-1 of complete graphs Kn:

d11 = 0 bd-1ii = n - 2

dij = 1 bd-1ij = -1

The constant is b = 1/(1-n). The inverse distance matrix of the complete graph is thus related to its Laplace-Kirchhoff matrix simply as

D-1K = 1/(1-n)STSK - I

(ii) D-1 of star graphs Sn rooted in the first vertex:

dii = 0 bd-1ii = 4(n - 2)

di1 = d1j = 1 bd-1ii = n -2, otherwise

dij = 2, otherwise d-1i1 = d-11j = -2

d-1ij =-1, otherwise

The constant is b = 1/2 (1-n). The inverse distance matrix of the star graph can be written (except the element d-1ij) as bD-1 = STS + (n-2)I - JJT.

(iii) D-1 of linear chains Ln:

d-1ij = i - j bd-111 = bd-1nn = n-2; bd-1ii = 2(n-1), otherwise

bd-1i,i +/-1 = 1-n; bd-11n = bd-1n1 = -1; d-1ij = 0.

The constant is b = 1/[2(1-n)]. The inverse of the topological distance matrix of the linear chain can be formulated again as its perturbed Laplace-Kirchhoff matrix

DL-1 = -1/2STSL + bX.

where X has elements x11 = x1n = xn1 = xnn = 1, xij = 0 otherwise. For short chains, the perturbed matrix is similar to the Laplace-Kirchhoff matrix of a cycle, but for infinite chains b goes to 0 and the perturbation X needed to destroy the singularity of STS is negligible.

(iv) DC-1 of an odd-membered cycle Cn for the shorter path is

d-1ij = min |i -j| mod n/2 bd-1ii = 1 -2p2

n = 2p + 1; bd-1i,i +p = 1 +p - p2; b d-1ij = n, otherwise;

The constant is b = 1/(p2 + p).The inverse distance matrix of odd-membered cycles can be expressed again as the sum of matrices

D-1C = nJJT - (p2 +p)PTSTSCP

where P is an unit permutation matrix.

For distance matrices of graphs with multiple bonds, defined by Balaban [15] and of molecules with heteroatoms [16], relations were much more complicated.

Discussion

To find a proof that the distance matrix of a tree is a multiple of an inner inverse of its quadratic form of incidence matrix took as many minutes as elapsed years when I did not suspect that such a relation could exist. I found it from a curiosity, realizing that the elements of corresponding Eichinger matrices E are distances. Rutherford discovered the relation before me [10], solving the classical Kirchhoff problem of spanning trees of electrical circuits formed by electrons in crystals. This paper was written simultaneously with [12], unfortunately it was lost by post and was idle. Klein and Randic were more general, but my proof, yielding the Wiener number W for an arbitrary constant c, could be interesting for chemistry and shows a specific role of the Eichinger matrices between the generalized inverses of STS. The constant c is not as arbitrary, as can be deduced from formal relations.

Finding of the generalized inverses of E using its complementary graph matrix, indicated shortly above, is possible probably by a relation of eigenvalues of the Laplace-Kirchhoff matrices both graphs, G and GC, which are complementary, too.

Eichinger introduced matrices E for linear chains only, as matrices transforming the quadratic form SST of the complete graph into the quadratic form WWT, where W is the walk or path matrix [17]. But this matrix is simultaneously the walk matrix of the linear chain WL [17] and because the incidence matrix of the complete graph can be split into the product SK = WL SL, it leads to formal equivalencies

SKESK-1= W S ESTWTL= WWTL or S ESTL= In-1

The relations between different matrices can be interpreted as follows [18]: A structure, characterized by its incidence matrix S, projects into the Hilbert space as two quadratic forms STS and SST. Their traces, thus sums of their eigenvalues, are equivalent to the original vector S. Some physical and chemical properties depend directly on eigenvalues of both quadratic forms, other ones only on the eigenvalues of the off-diagonal adjacency matrix A. Other physical properties depend on the inverse eigenvalues or elements of inverse matrices, which for acyclic graphs are distances [9]. The Laplace-Kirchhoff matrices are singular, they have one zero eigenvalue. But they can be perturbed, meaning that a slight distortion of all their elements leads to nonsingular matrices with true inverses. Such a perturbation can be produced for example by the electrical potential, applied to a circuit [12].

The situation is complicated by embedding of molecules into the three dimensional space. Topological distances must be replaced by geometrical ones (or resistance ones), which are squares of Euclidean distances, to be comparable with topological distance matrices [19,20]. The conformation of the graph is changed. Different distance moments have different properties, which depend on symmetry.

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