New particlelike solutions
in modified gravity:
the Higgs monopoles
André Füzfa
Massimiliano Rinaldi & Sandrine Schlögel
Namur Center for Complex Systems - naXys
University of Namur
Eventuellement suivi de
«!A n’ouvrir qu’en cas de Prix Nobel!»
SOME PARTICLELIKE SOLUTIONS
IN CLASSICAL FIELD THEORY
Part One
Why particlelike solutions?
!   Original motivation:
Temptative models of elementary particles such as
electron in terms of solutions to classical field equations
Naive view since no quantum mechanical aspects…
!Regularization of singularities in classical field
theory for point sources (spherical symmetry)
!   Alternatives to black holes
Black holes: singular solutions
classical regularisation of gravitational singularities
new candidates for compact objects (high-energy
astrophysical sources such as quasars, galactic centers,
etc.)
What makes a particlelike solution?
!Spherical symmetry
!Static (Time-independent) equilibrium configurations
!Globally regular (no singularities at r=0 and r->)
!Asymptotically flat: vanishing forces at spatial infinity
!Finite-energy/mass
!   Stable under perturbations (when possible)
An example in electromagnetism
!   Electron: some electrical charge distribution, pointlike at
distance
!Which electric potential? => Maxwell equations
For static potential : Poisson equation
V’’r+2V’=0 ; (.)’=d(.)/dr
Distance
The solution V(r) ~ 1/r is singular!
Electric potential
Particlelike solution
Inner
region,
regularity
at r=0
Outer region:
fast decrease when r->
So that total energy is bounded
Electron radius
Naive
classical
vision!
Quantum
Mechanics!
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