activity
20052025
most citedProspects for Fundamental Physics with LISA

401 citations · 1.2k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.GA2025

Effective supernova dust yields from rotating and non-rotating stellar progenitors

Koki Otaki, Raffaella Schneider, Luca Graziani +4

Supernovae (SNe) are believed to be the dominant sources of dust production at high redshift. However, the reverse shock generated by the interaction of the SN forward shock and th…

astro-ph.GA2020★ 23 cited

Seeding the second star -- II. CEMP star formation enriched from faint supernovae

Gen Chiaki, John H. Wise, Stefania Marassi +3

Carbon-enhanced metal-poor (CEMP) stars are the living fossils holding records of chemical enrichment from early generations of stars. In this work, we perform a set of numerical s…

gr-qc2020★ 401 cited

Prospects for Fundamental Physics with LISA

Enrico Barausse, Emanuele Berti, Thomas Hertog +318

In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental…

astro-ph.HE2019★ 20 cited

Binary white dwarfs and decihertz gravitational wave observations: From the Hubble constant to supernova astrophysics

Andrea Maselli, Stefania Marassi, Marica Branchesi

Coalescences of binary white dwarfs represent a copious source of information for gravitational wave interferometers operating in the decihertz band. Moreover, according to the dou…

astro-ph.GA2019★ 19 cited

Evolution of dwarf galaxies hosting GW150914-like events

S. Marassi, L. Graziani, M. Ginolfi +4

Here we present a detailed analysis of the properties and evolution of different dwarf galaxies, candidate to host the coalescence of black hole binary systems (BHB) generating GW1…

astro-ph.SR2018★ 56 cited

Supernova dust yields: the role of metallicity, rotation, and fallback

S. Marassi, R. Schneider, M. Limongi +3

Supernovae (SNe) are considered to have a major role in dust enrichment of high redshift galaxies and, due to the short lifetimes of interstellar grains, in dust replenishment of l…