pith. sign in

Francesco Pace

Identifiers

  • name variant Francesco Pace 0.60 · backfill

Papers (33)

  1. How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity astro-ph.CO · 2026 · author #4
  2. The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics astro-ph.CO · 2025 · author #183
  3. Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies astro-ph.CO · 2022 · author #142
  4. Cosmologically viable generalized Einstein-Aether theories astro-ph.CO · 2018 · author #2
  5. Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model astro-ph.GA · 2018 · author #2
  6. A Data-Driven Approach to Dynamically Adjust Resource Allocation for Compute Clusters cs.DC · 2018 · author #1
  7. Gravitational wave constraints on dark sector models astro-ph.CO · 2018 · author #2
  8. Do cosmological data rule out $f(\mathcal{R})$ with $w\neq-1$? astro-ph.CO · 2017 · author #3
  9. On the implementation of the spherical collapse model for dark energy models astro-ph.CO · 2017 · author #1
  10. Stocator: A High Performance Object Store Connector for Spark cs.DC · 2017 · author #6
  11. Cosmological perturbation theory in Generalized Einstein-Aether models astro-ph.CO · 2017 · author #2
  12. A high precision semi-analytic mass function astro-ph.CO · 2017 · author #2
  13. Shear and vorticity in the spherical collapse of dark matter haloes astro-ph.CO · 2016 · author #2
  14. Effects of tidal gravitational fields in clustering dark energy models astro-ph.CO · 2016 · author #1
  15. Flexible Scheduling of Distributed Analytic Applications cs.DC · 2016 · author #1
  16. Constraints on shear and rotation with massive galaxy clusters astro-ph.CO · 2016 · author #2
  17. Approximation of the potential in scalar field dark energy models astro-ph.CO · 2016 · author #2
  18. Spherical collapse of dark matter haloes in tidal gravitational fields astro-ph.CO · 2016 · author #2
  19. Experimental Performance Evaluation of Cloud-Based Analytics-as-a-Service cs.DC · 2016 · author #1
  20. Effects of ghost dark energy perturbations on the evolution of spherical overdensities gr-qc · 2015 · author #3
  21. Constraints on $\Omega_\mathrm{m}$ and $\sigma_8$ from the potential-based cluster temperature function astro-ph.CO · 2015 · author #2
  22. The importance of the cosmic web and halo substructure for power spectra astro-ph.CO · 2015 · author #1
  23. Intrinsic size correlations in weak lensing astro-ph.CO · 2014 · author #3
  24. Evolution of spherical overdensities in holographic dark energy models gr-qc · 2014 · author #3
  25. Can observational growth rate data favour the clustering dark energy models? astro-ph.CO · 2014 · author #3
  26. Raytracing simulations of coupled dark energy models astro-ph.CO · 2014 · author #1
  27. Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities astro-ph.CO · 2013 · author #1
  28. Bounded Scalar Perturbations in Bouncing Brane World Cosmologies gr-qc · 2013 · author #2
  29. A comparison of structure formation in minimally and non-minimally coupled quintessence models astro-ph.CO · 2013 · author #1
  30. Extended Spherical Collapse and the Accelerating Universe astro-ph.CO · 2012 · author #2
  31. Relativistic virialization in the Spherical Collapse model for Einstein-de Sitter and \Lambda CDM cosmologies astro-ph.CO · 2012 · author #2
  32. Strong lensing in the MareNostrum Universe: biases in the cluster lens population astro-ph.CO · 2010 · author #3
  33. Arc sensitivity to cluster ellipticity, asymmetries and substructures astro-ph · 2006 · author #3

Mentions

  • 1310.5319 #1 · backfill · confidence 0.70 Francesco Pace
  • 1310.5038 #2 · backfill · confidence 0.70 Francesco Pace
  • 1307.7026 #1 · backfill · confidence 0.70 Francesco Pace
  • 1207.5789 #2 · backfill · confidence 0.70 Francesco Pace
  • 1206.0618 #2 · backfill · confidence 0.70 Francesco Pace
  • 1003.4544 #3 · backfill · confidence 0.70 Francesco Pace

Frequent Coauthors