Past member · PhD Student
Clemente Smarra
Former PhD student at SISSA (2022–2025), supervised by the node PI. Worked on the pulsar-timing-array stochastic background, including the imprint of supermassive black hole scalarization and the four-point correlator as a probe of non-Gaussianity. His papers in this area acknowledge GWSky.
Pulsar timing arraysStochastic gravitational-wave backgroundsScalar-tensor gravity
Papers
- Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator
A. Kuntz, C. Smarra, M. Vaglio · arXiv:2603.12311 · Phys. Rev. D 114, 084020 (2026)
- Probing supermassive black hole scalarization with pulsar timing arrays
C. Smarra, L. Capuano, A. Kuntz · arXiv:2505.20402 · Phys. Rev. D 112, 064005 (2025)