TY - JOUR
T1 - Superexpansionary divergence
T2 - Breakdown of perturbative quantum field theory in spacetime with accelerated expansion
AU - Sasaki, M.
AU - Suzuki, H.
AU - Yamamoto, K.
AU - Yokoyama, J.
PY - 1993
Y1 - 1993
N2 - The authors show that perturbative quantum field theory may break down in curved spacetime with accelerated expansion. They consider lambda phi p-theory (p=3,4,5,. . .) with curvature coupling xi R phi 2 in de Sitter space and perturbatively evaluate the n-point function. They find the vertex integral over all spacetime points diverges for a certain range of the mass and curvature coupling. In particular, for lambda phi 4 theory with xi =0, the divergence arises for m2/H 227/16 where H-1 is the de Sitter radius. Then, they show that the same type of divergence arises quite generally in a spacetime with accelerated expansion. Since it is caused by unboundedly accelerated expansion of spacetime, they call it the superexpansionary divergence.
AB - The authors show that perturbative quantum field theory may break down in curved spacetime with accelerated expansion. They consider lambda phi p-theory (p=3,4,5,. . .) with curvature coupling xi R phi 2 in de Sitter space and perturbatively evaluate the n-point function. They find the vertex integral over all spacetime points diverges for a certain range of the mass and curvature coupling. In particular, for lambda phi 4 theory with xi =0, the divergence arises for m2/H 227/16 where H-1 is the de Sitter radius. Then, they show that the same type of divergence arises quite generally in a spacetime with accelerated expansion. Since it is caused by unboundedly accelerated expansion of spacetime, they call it the superexpansionary divergence.
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U2 - 10.1088/0264-9381/10/5/003
DO - 10.1088/0264-9381/10/5/003
M3 - Article
AN - SCOPUS:21344474307
SN - 0264-9381
VL - 10
SP - L55-L60
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
IS - 5
M1 - 003
ER -