Orbital Chromatic and Flow Roots

  • Authors:
  • PETER J. CAMERON;K. K. KAYIBI

  • Affiliations:
  • School of Mathematical Sciences, Queen Mary, University of London, Mile End Road, London E1 4NS, UK (e-mail: P.J.Cameron@qmul.ac.uk/ kokokayibi@yahoo.co.uk);School of Mathematical Sciences, Queen Mary, University of London, Mile End Road, London E1 4NS, UK (e-mail: P.J.Cameron@qmul.ac.uk/ kokokayibi@yahoo.co.uk)

  • Venue:
  • Combinatorics, Probability and Computing
  • Year:
  • 2007

Quantified Score

Hi-index 0.00

Visualization

Abstract

The chromatic polynomial PΓ(x) of a graph“ is a polynomial whose value at the positive integerk is the number of proper k-colourings of Γ. IfG is a group of automorphisms of Γ, then there is apolynomial OPΓ,G(x), whose value atthe positive integer k is the number of orbits of Gon proper k-colourings of “.It is known that real chromatic roots cannot be negative, butthey are dense in [32/27·∞). Here we discuss thelocation of real orbital chromatic roots. We show, for example,that they are dense in ℝ, but under certain hypotheses, thereare zero-free regions.We also look at orbital flow roots. Here things are morecomplicated because the orbit count is given by a multivariatepolynomial; but it has a natural univariate specialization, and weshow that the roots of these polynomials are dense in the negativereal axis.