Lattice Quantum Gravity and Asymptotic Safety
Jack Laiho
Syracuse University
Lattice Quantum Gravity and Asymptotic Safety Jack Laiho Syracuse - - PowerPoint PPT Presentation
Lattice Quantum Gravity and Asymptotic Safety Jack Laiho Syracuse University April 22, 2016 Quantum Gravity Understanding quantum gravity is one of the outstanding problems in theoretical physics. Straightforward implementation as a
Syracuse University
◮ Straightforward implementation as a perturbative quantum field theory is
◮ Explicitly confirmed that a counter-term is necessary at 2-loop order for
◮ Can be formulated as an effective field theory at low energies, but new
◮ Effective field theory arguments suggest cosmological constant should
◮ Gravity is effectively renormalizable when formulated non-perturbatively.
◮ Renormalization group flows of couplings have a non-trivial fixed point,
◮ In a Euclidean lattice formulation the fixed point would show up as a
◮ Euclidean dynamical triangulations (EDT) is a lattice formulation that
◮ In lattice gravity, the lattice itself is a dynamical entity, which evolves in
◮ EDT works perfectly in 2d, where it reproduces the results of non-critical
◮ The EDT formulation in 4d was shown to have two phases, a “crumpled"
N2
j=1
◮ Key new idea is that a fine-tuning of bare parameters in EDT is
◮ Previous work did not implement this fine-tuning, leading to negative
◮ For gauge theories this is equivalent to the gauge symmetry; ensures
◮ For reparameterization invariant theories, canonical symmetry is closely
◮ Canonical symmetry and diff invariance are equivalent up to classical
◮ Dynamical triangulations is diffeomorphism invariant. In 2d, EoM are
◮ The Metropolis Algorithm is implemented using a set of local update
◮ We introduce a new algorithm for parallelizing the code, which we call
β Branched Polymer Phase Collapsed Phase κ2 B A D C Crinkled Region
κ β
◮ Must show recovery of semiclassical physics in 4 dimensions. ◮ Must show existence of continuum limit at 2nd order critical point. ◮ Argument against renormalizability of gravity due to Banks. Tension
d−1 d ,
d−2 d−3 .
4k 8k 16k
β=1.5 β=0 β=-0.6 β = -0.8
100 200 300 400 500 σ 0.01 0.02 0.03 0.04 0.05 0.06 P(σ)
β=-0.8 β=-0.6 β=0 β=0.8 β=1.5
100 200 300 400 500 σr 0.01 0.02 0.03 0.04 0.05 0.06 P(σr)
β=−0.8 β=-0.6 β=0 β=0.8 β=1.5
500 1000 1500 2000 σ 0.5 1 1.5 2 2.5 3 3.5 4 DS(σ)
8k
0.05 0.1 0.15 0.2 0.25 1/V 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 DS(V,a)
β=0 β=0.8 β=1.5
0.05 0.1 0.15 0.2 0.25 1/V 0.5 1 1.5 2 2.5 3 DS(V,a)
β=1.5 β=0.8 β=0
d−1 d ,
d−2 d−3 ,
sub x 10