Per Kraus
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Per Kraus has a total of 27 co-authors. Here are the top co-authors by number of shared publications:
- Eric Perlmutter
Department of Physics and Astronomy University of California 90095 Los Angeles CA USA
9 shared publications - Eric D'Hoker
Mani L. Bhaumik Institute for Theoretical Physics Department of Physics and Astronomy University of California 90095 Los Angeles CA USA
8 shared publications - Eliot Hijano
University of California
6 shared publications - Martin Ammon
Friedrich-Schiller-Universität, Jena, Germany
5 shared publications - Michael Gutperle
University of California Los Angeles
5 shared publications - Finn Larsen
University of Michigan
4 shared publications
Latest Publications
- Open Access
- 26 April 2023
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2023 (4) , 1-58
Systematics of boundary actions in gauge theory and gravity
- 26 April 2023
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2023 (4) , 1-58
Open AccessSystematics of boundary actions in gauge theory and gravity
- Open Access
- 24 October 2020
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2020 (10) , 1-35
Anomalous dimensions from thermal AdS partition functions
- 24 October 2020
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2020 (10) , 1-35
Open AccessAnomalous dimensions from thermal AdS partition functions
- Open Access
Anomalous Dimensions from Thermal AdS Partition Functions
We develop an efficient method for computing thermal partition functions of weakly coupled scalar fields in AdS. We consider quartic contact interactions and show how to evaluate the relevant two-loop vacuum diagrams without performing any explicit AdS integration, the key step being the use of Kallen-Lehmann type identities. This leads to a simple method for extracting double-trace anomalous dimensions in any spacetime dimension, recovering known first-order results in a streamlined fashion.
Open AccessAnomalous Dimensions from Thermal AdS Partition Functions
We develop an efficient method for computing thermal partition functions of weakly coupled scalar fields in AdS. We consider quartic contact interactions and show how to evaluate the relevant two-loop vacuum diagrams without performing any explicit AdS integration, the key step being the use of Kallen-Lehmann type identities. This leads to a simple method for extracting double-trace anomalous dimensions in any spacetime dimension, recovering known first-order results in a streamlined fashion.
- Top Cited PapersOpen Access
- 20 January 2020
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2020 (1) , 1-16
Semi-classical Virasoro blocks: proof of exponentiation
Virasoro conformal blocks are expected to exponentiate in the limit of large central charge c and large operator dimensions h i , with the ratios h i /c held fixed. We prove this by employing the oscillator formulation of the Virasoro algebra and its representations. The techniques developed are then used to provide new derivations of some standard results on conformal blocks.
- 20 January 2020
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2020 (1) , 1-16
Top Cited PapersOpen AccessSemi-classical Virasoro blocks: proof of exponentiation
Virasoro conformal blocks are expected to exponentiate in the limit of large central charge c and large operator dimensions h i , with the ratios h i /c held fixed. We prove this by employing the oscillator formulation of the Virasoro algebra and its representations. The techniques developed are then used to provide new derivations of some standard results on conformal blocks.
- Open Access
Gravitational Wilson lines in AdS$_{\bf 3}$
The construction of gravitational Wilson lines in the Chern-Simons formulation of $AdS_3$ gravity in terms of composite operators in the dual boundary conformal field theory is reviewed. New evidence is presented that the Wilson line, dimensionally regularized and suitably renormalized, behaves as a bi-local operator of two conformal primaries whose dimension is predicted by SL(2,R) current algebra.Open AccessGravitational Wilson lines in AdS$_{\bf 3}$
The construction of gravitational Wilson lines in the Chern-Simons formulation of $AdS_3$ gravity in terms of composite operators in the dual boundary conformal field theory is reviewed. New evidence is presented that the Wilson line, dimensionally regularized and suitably renormalized, behaves as a bi-local operator of two conformal primaries whose dimension is predicted by SL(2,R) current algebra. - Open Access
Semi-classical Virasoro blocks: proof of exponentiation
Virasoro conformal blocks are expected to exponentiate in the limit of large central charge $c$ and large operator dimensions $h_i$, with the ratios $h_i/c$ held fixed. We prove this by employing the oscillator formulation of the Virasoro algebra and its representations. The techniques developed are then used to provide new derivations of some standard results on conformal blocks.Open AccessSemi-classical Virasoro blocks: proof of exponentiation
Virasoro conformal blocks are expected to exponentiate in the limit of large central charge $c$ and large operator dimensions $h_i$, with the ratios $h_i/c$ held fixed. We prove this by employing the oscillator formulation of the Virasoro algebra and its representations. The techniques developed are then used to provide new derivations of some standard results on conformal blocks. - 1 January 2018
- Published by Elsevier in Annals of Physics
- Vol. 388, 135-146
Can a quantum critical state represent a blackbody?
- 1 January 2018
- Published by Elsevier in Annals of Physics
- Vol. 388, 135-146
Can a quantum critical state represent a blackbody?
- Open Access
- 31 May 2017
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2017 (5) , 1-22
A cardy formula for three-point coefficients or how the black hole got its spots
- 31 May 2017
- Published by Springer Nature in Journal of High Energy Physics
- Vol. 2017 (5) , 1-22
Open AccessA cardy formula for three-point coefficients or how the black hole got its spots
- Open Access
Can a quantum critical state represent a blackbody?
The blackbody theory of Planck played a seminal role in the development of quantum theory at the turn of the past century. A blackbody cavity is generally thought to be a collection of photons in thermal equilibrium; the radiation emitted is at all wavelengths, and the intensity follows a scaling law, which is Planck's characteristic distribution law. These photons arise from non-interacting normal modes. Here we suggest that certain quantum critical states when heated emit "radiation" at all wavelengths and satisfy all the criteria of a blackbody. An important difference is that the "radiation" does not necessarily consist of non-interacting photons, but also emergent relativistic bosons or fermions. The examples we provide include emergent relativistic fermions at a topological quantum critical point. This perspective on a quantum critical state may be illuminating in many unforeseen ways.
Open AccessCan a quantum critical state represent a blackbody?
The blackbody theory of Planck played a seminal role in the development of quantum theory at the turn of the past century. A blackbody cavity is generally thought to be a collection of photons in thermal equilibrium; the radiation emitted is at all wavelengths, and the intensity follows a scaling law, which is Planck's characteristic distribution law. These photons arise from non-interacting normal modes. Here we suggest that certain quantum critical states when heated emit "radiation" at all wavelengths and satisfy all the criteria of a blackbody. An important difference is that the "radiation" does not necessarily consist of non-interacting photons, but also emergent relativistic bosons or fermions. The examples we provide include emergent relativistic fermions at a topological quantum critical point. This perspective on a quantum critical state may be illuminating in many unforeseen ways.
- Open Access
Nature abhors a horizon
The information paradox can be resolved if we recognize that the wavefunctional in gravity $\Psi[g]$ should be considered on the {\it whole} of superspace, the space of possible $g$. The largeness of the Bekenstein entropy implies a vast space of gravitational solutions, which are conjectured to be fuzzball configurations. In the WKB approximation, the wavefunctional for a collapsing shell is oscillatory in a small region of superspace, and the classical approximation picks out this part. But the wavefunctional will be damped (`under the barrier') in the remainder of this vast superspace. We perform a simple computation to show that at the threshold of black hole formation, the barrier is lowered enough to make the latter part oscillatory; this alters the classical evolution and avoids horizon formation.Open AccessNature abhors a horizon
The information paradox can be resolved if we recognize that the wavefunctional in gravity $\Psi[g]$ should be considered on the {\it whole} of superspace, the space of possible $g$. The largeness of the Bekenstein entropy implies a vast space of gravitational solutions, which are conjectured to be fuzzball configurations. In the WKB approximation, the wavefunctional for a collapsing shell is oscillatory in a small region of superspace, and the classical approximation picks out this part. But the wavefunctional will be damped (`under the barrier') in the remainder of this vast superspace. We perform a simple computation to show that at the threshold of black hole formation, the barrier is lowered enough to make the latter part oscillatory; this alters the classical evolution and avoids horizon formation.