Without any regards to the physics or the geometry used to generate this result, let's examine the formula of Gukov (see p. 32):
ISU(2)(q,t)=12∑m∈Z∫dz2πizz2pmt−2mq−2|m|(1−z±2q|m|)×(1/t;q)∞(z±2q|m|/t;q)∞(qt;q)∞(z±2q|m|+1t;q)∞
The standard notation (for those who use it) is that
z± is a shorthand:
f(z±2)=f(z2)f(z−2)
While there is element of sarcasm, here this is a real honest-to-goodness superconformal index computation, taken from a serious physics paper. My impression is we spend the good part of 19th century ascribing meaning to q-series like these and some of them turned out to have good modular properties.
For now there is basic property:
I(q,t)∈Z[t][[q]]
This is the Lens space index. Let
M3=L(p,1)≃S3/Zp, this has to do with:
- N=2 Chern-Simons theory (so it is possibly supersymmetric)
- The theory is also called T[L(p,1),SU(2)]
This post imported from StackExchange MathOverflow at 2017-11-03 22:20 (UTC), posted by SE-user john mangual