Free boson formulation of boundary states in W_3 minimal models and the critical Potts model

ArXiv hep-th/0306082 (2003)

Authors:

Alexandre F Caldeira, Shinsuke Kawai, John F Wheater

Abstract:

We develop a Coulomb gas formalism for boundary conformal field theory having a $W$ symmetry and illustrate its operation using the three state Potts model. We find that there are free-field representations for six $W$ conserving boundary states, which yield the fixed and mixed physical boundary conditions, and two $W$ violating boundary states which yield the free and new boundary conditions. Other $W$ violating boundary states can be constructed but they decouple from the rest of the theory. Thus we have a complete free-field realization of the known boundary states of the three state Potts model. We then use the formalism to calculate boundary correlation functions in various cases. We find that the conformal blocks arising when the two point function of $\phi_{2,3}$ is calculated in the presence of free and new boundary conditions are indeed the last two solutions of the sixth order differential equation generated by the singular vector.

Free boson formulation of boundary states in W_3 minimal models and the critical Potts model

(2003)

Authors:

Alexandre F Caldeira, Shinsuke Kawai, John F Wheater

Extending QCD perturbation theory to higher energies

(2003)

Authors:

M Ciafaloni, D Colferai, GP Salam, AM Stasto

The clustering of ultra-high energy cosmic rays and their sources

Phys.Rev.D 67 (2003) 103005-103005

Authors:

NW Evans, F Ferrer, S Sarkar

Abstract:

The sky distribution of cosmic rays with energies above the 'GZK cutoff' holds important clues to their origin. The AGASA data, although consistent with isotropy, shows evidence for small-angle clustering, and it has been argued that such clusters are aligned with BL Lacertae objects, implicating these as sources. It has also been suggested that clusters can arise if the cosmic rays come from the decays of very massive relic particles in the Galactic halo, due to the expected clumping of cold dark matter. We examine these claims and show that both are in fact not justified.

Theory and phenomenology of non-global logarithms

ArXiv hep-ph/0305232 (2003)

Authors:

RB Appleby, GP Salam

Abstract:

We discuss the theoretical treatment of non-global observables, those quantities that are sensitive only to radiation in a restricted region of phase space, and describe how large `non-global' logarithms arise when we veto the energy flowing into the restricted region. The phenomenological impact of non-global logarithms is then discussed, drawing on examples from event shapes in DIS and energy-flow observables in 2-jet systems. We then describe techniques to reduce the numerical importance of non-global logarithms, looking at clustering algorithms in energy flow observables and the study of associated distribution of multiple observables.