Bargmann transform


The Bargmann transform of a function, f, is a linear map B:X⁢(ℝ)→Y⁢(ℂ) defined by

B⁢f⁢(z)=2⁢∫ℝf⁢(t)⁢e2⁢π⁢t⁢z-π⁢t2-π2⁢z2⁢𝑑t
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