English

The C-Numerical Range for Schatten-Class Operators

Functional Analysis 2023-03-30 v3

Abstract

We generalize the CC-numerical range WC(T)W_C(T) from trace-class to Schatten-class operators, i.e. to CBp(H)C\in\mathcal B^p(\mathcal H) and TBq(H)T\in\mathcal B^q(\mathcal H) with 1/p+1/q=11/p + 1/q = 1, and show that its closure is always star-shaped with respect to the origin. For q(1,]q \in (1,\infty], this is equivalent to saying that the closure of the image of the unitary orbit of TBq(H)T\in\mathcal B^q(\mathcal H) under any continous linear functional L(Bq(H))L\in(\mathcal B^q(\mathcal H))' is star-shaped with respect to the origin. For q=1q=1, one has star-shapedness with respect to tr(T)We(L)\operatorname{tr}(T)W_e(L), where We(L)W_e(L) denotes the essential range of LL. Moreover, the closure of WC(T)W_C(T) is convex if CC or TT is normal with collinear eigenvalues. If CC and TT are both normal, then the CC-spectrum of TT is a subset of the CC-numerical range, which itself is a subset of the closure of the convex hull of the CC-spectrum. This closure coincides with the closure of the CC-numerical range if, in addition, the eigenvalues of CC or TT are collinear.

Keywords

Cite

@article{arxiv.1808.06898,
  title  = {The C-Numerical Range for Schatten-Class Operators},
  author = {Gunther Dirr and Frederik vom Ende},
  journal= {arXiv preprint arXiv:1808.06898},
  year   = {2023}
}

Comments

12 pages; extended version of the Addendum (linked in DOI) to a previous article (arXiv:1712.01023)

R2 v1 2026-06-23T03:39:29.188Z