Question

Three principal invariants with respect to this quantity are named for Chern-Pontryagin, Euler, and Kretschmann. A renormalization method named for this quantity is used to find the order parameter of topological phase transitions. Non-zero values of this quantity necessitate generalizing the derivative operator to the (*) covariant derivative. The affine connections vanish (10[1])for systems in which this quantity is equal to zero. The contracted Bianchi identity relates a tensor and a scalar describing this property, both of which are named for Ricci. Non-zero (10[1])values (10[2])of this quantity cause gravitational lensing, or the bending of light. When this quantity is non-zero, straight lines are generalized into geodesics. For 10 points, what quantity is zero for flat spacetime? ■END■

ANSWER: curvature [or curvature invariants; or curvature renormalization group method; or Ricci curvature; or curvature of spacetime]
<Leo Law, Physics>
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Buzzes

PlayerTeamOpponentBuzz PositionValue
Colin VeeversLibrary of Babel School of Continuing StudiesWaterloo Hatsune5010
Ian ChowLa Clique du ChateauWaterloo Miku8110
Jason ZhangToronto RoflMixed-Affiliated Contingency, Off the Team & Absent: Wong, Adrian8210
Sky LiToronto WearyToronto Joy8210

Summary

2023 Penn Bowl (Harvard)10/21/2023Y2100%0%0%84.50
2023 Penn Bowl (Mainsite)10/21/2023Y786%0%29%69.17
2023 Penn Bowl (Norcal)10/28/2023Y2100%0%0%46.50
2023 Penn Bowl (South Central)10/28/2023Y367%0%33%113.50
2023 Penn Bowl (UK)10/28/2023Y5100%0%0%68.20
2023 Penn Bowl @ Waterloo10/28/2023Y4100%0%0%73.75
2023 Penn Bowl @ UNC10/28/2023Y3100%0%0%70.67
2023 Penn Bowl @ FSU10/28/2023Y1100%0%0%80.00