Bargmann transform
The Bargmann transform of a function, f, is a linear map B:X(ℝ)→Y(ℂ) defined by
Bf(z)=√2∫ℝf(t)e2πtz-πt2-π2z2𝑑t |
Theorem.
The Bargmann transform on L2(R), B:L2(R)→F2(C), is a unitary transformation. Here F2(C) is the Fock space.
References
- 1 Karlheinz Gröchenig, ”Foundations of Time-Frequency Analysis,” Birkhhäuser (2000)
Title | Bargmann transform |
---|---|
Canonical name | BargmannTransform |
Date of creation | 2013-03-22 16:44:45 |
Last modified on | 2013-03-22 16:44:45 |
Owner | ErlendA (6587) |
Last modified by | ErlendA (6587) |
Numerical id | 7 |
Author | ErlendA (6587) |
Entry type | Definition |
Classification | msc 43A15 |
Defines | Bargmann transform |