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- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoIT850 papers
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- Sapienza University of RomeIT442 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR429 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT412 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PadovaIT406 papers
- University of Naples Federico IIIT394 papers
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145 papers · 1 filter
Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
Jasbir Singh, Paola Severgnini, Vieri Cammelli +10
With the upcoming space- and Moon-based gravitational-wave detectors, LISA and LGWA respectively, a new era of GW astronomy will begin with the possibility of detections of the mer…
Requirements on bandpass resolution and measurement precision for LiteBIRD
S. Giardiello, A. Carones, T. Ghigna +95
In this work, we study the impact of an imperfect knowledge of the instrument bandpasses on the estimate of the tensor-to-scalar ratio in the context of the next-generation Lit…
Non-Gaussianity of Tensor Induced Density Perturbations
Mariam Abdelaziz, Pritha Bari, Sabino Matarrese +1
We investigate the non-Gaussianity of second-order matter density perturbations induced by primordial gravitational waves (GWs). These tensor-induced scalar modes arise from local…
Non-linear effects on the Cosmological Gravitational Wave Background anisotropies
Alina Mierna, Sabino Matarrese, Nicola Bartolo +1
The Cosmological Gravitational Wave Background (CGWB) anisotropies contain valuable information about the physics of the early universe. Given that General Relativity is intrinsica…
Constraints on self-interaction cross-sections of dark matter in universal bound states from direct detection
The CRESST Collaboration
Lambda- Cold Dark Matter (LambdaCDM) has been successful at explaining the large-scale structures in the universe but faces severe issues on smaller scales when compared to observa…
Superfluid dark stars
Lorenzo Cipriani, Massimo Mannarelli, Fabrizio Nesti +1
We present a superfluid dark star model consisting of relativistic dark bosons with two-body self-interaction. The obtained masses, radii, and tidal deformability depend in a simpl…