Giacomo Ferrante

ORCID: 0000-0003-0487-7195
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About
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Research Areas
  • Cosmology and Gravitation Theories
  • Black Holes and Theoretical Physics
  • Dark Matter and Cosmic Phenomena
  • Galaxies: Formation, Evolution, Phenomena
  • Pulsars and Gravitational Waves Research
  • Sports Performance and Training
  • Exercise and Physiological Responses
  • Thermoregulation and physiological responses
  • Particle physics theoretical and experimental studies

Université de Montpellier
2023-2024

Centre National de la Recherche Scientifique
2023-2024

Laboratoire Univers et Particules de Montpellier
2024

Sapienza University of Rome
2023

University of Padua
2021

The authors develop a formalism for computing the abundance of primordial black holes (PBH) in presence local non-Gaussianities curvature perturbation field. They show that polynomial expansions will not suffice certain limits and provide numerical methods to address this issue. demonstrate how their technique affects both total PBH abundances gravitational wave expectations.

10.1103/physrevd.107.043520 article EN Physical review. D/Physical review. D. 2023-02-16

We revise primordial black holes (PBHs) production in the axion-curvaton model, light of recent developments computation their abundance accounting for non-gaussianities (NGs) curvature perturbation up to all orders. find that NGs intrinsically generated such scenarios have a relevant impact on phenomenology associated PBHs and, particular, relation between and signal second-order gravitational waves. show this model could explain both totality dark matter asteroid mass range tentative...

10.1088/1475-7516/2023/06/057 article EN cc-by Journal of Cosmology and Astroparticle Physics 2023-06-01

A bstract In models with spontaneous symmetry breaking by scalar fields in large group representations, we observe that some of the masses can be loop-suppressed respect to naive expectation from selection rules. We present minimal — SU(2) five-plet and SU(3) ten-plet such accidentally light scalars, featuring compact tree-level flat directions lifted radiative corrections. sketch potential applications, stable relics slow roll cosmology, hierarchy fine-tuning problems particle physics.

10.1007/jhep01(2024)075 article EN cc-by Journal of High Energy Physics 2024-01-15

We construct a hybrid-inflation model where the inflaton potential is generated radiatively, as gauge symmetries guarantee it to be accidentally flat at tree level. The can regarded small-field version of natural inflation, with inflation ending when mass second scalar, waterfall field, turns tachyonic. This provides minimal, robust realization hybrid which predicts specific correlations among cosmic microwave background observables. Tachyonic preheating leads production gravitational waves...

10.1103/physrevd.110.103506 article EN Physical review. D/Physical review. D. 2024-11-08

The marathon is the most classic Olympic running event. In several cities worldwide it has become very popular with participation increasing during last 20 years, particularly by Master Athletes. There are evidences that long-distance could provide considerable health benefits for older runners, specifically risk reduction of cardiovascular diseases, cancer, diabetes, depression, and falls. Several studies have focused on distribution participants their performance famous marathons such as...

10.4081/ejtm.2021.10266 article EN cc-by-nc European Journal of Translational Myology 2021-11-10

We revise primordial black holes (PBHs) production in the axion-curvaton model, light of recent developments computation their abundance accounting for non-gaussianities (NGs) curvature perturbation up to all orders. find that NGs intrinsically generated such scenarios have a relevant impact on phenomenology associated PBHs and, particular, relation between and signal second-order gravitational waves. show this model could explain both totality dark matter asteroid mass range tentative...

10.48550/arxiv.2305.13382 preprint EN other-oa arXiv (Cornell University) 2023-01-01

We develop an exact formalism for the computation of abundance primordial black holes (PBHs) in presence local non-gaussianity (NG) curvature perturbation field. For first time, we include NG going beyond widely used quadratic and cubic approximations, consider a completely generic functional form. Adopting threshold statistics compaction function, address both narrow broad power spectra. While our formulas are generic, discuss explicit examples phenomenological relevance considering physics...

10.48550/arxiv.2211.01728 preprint EN other-oa arXiv (Cornell University) 2022-01-01
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