A Magnetized Strongly Turbulent Corona as the Source of Neutrinos from NGC 1068

Autor: Damiano F. G. Fiorillo, Luca Comisso, Enrico Peretti, Maria Petropoulou, Lorenzo Sironi

Publikováno v: The Astrophysical Journal, Vol 974, Iss 1, p 75 (2024)

The cores of active galactic nuclei are potential accelerators of 10–100 TeV cosmic rays, in turn producing high-energy neutrinos. This picture was confirmed by the compelling evidence of a TeV neutrino signal from the nearby active galaxy NGC 1068

Externí odkaz: https://doaj.org/article/5ad128f2c43c471696a0ea2b1f04d328

Strategies to Obtain Encapsulation and Controlled Release of Pentamidine in Mesoporous Silica Nanoparticles

Autor: Enrico Peretti, Ivana Miletto, Barbara Stella, Flavio Rocco, Gloria Berlier, Silvia Arpicco

Publikováno v: Pharmaceutics, Vol 10, Iss 4, p 195 (2018)

Pentamidine (PTM), an antiprotozoal agent used in clinics as pentamidine isethionate salt (PTM-S), recently showed high potential also for the treatment of cancer and myotonic dystrophy type I. However, a severe limit to the systemic administration o

Externí odkaz: https://doaj.org/article/d541f017b1ed4787b2377f656d4f6a56

Testing hadronic and photo-hadronic interactions as responsible for UHECR and neutrino fluxes from Starburst Galaxies

Autor: Antonio Condorelli, Denise Boncioli, Enrico Peretti, Sergio Petrera

We test the hypothesis of starburst galaxies as sources of ultra-high energy cosmic rays and high-energy neutrinos. The computation of interactions of ultra-high energy cosmic rays in the starburst environment as well as in the propagation to the Ear

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ad9325e5b4bad0962973b4d7baacb26
http://arxiv.org/abs/2209.08593

Particle acceleration in winds of star clusters

Autor: Giovanni Morlino, Enrico Peretti, P. Cristofari, P. Blasi

Publikováno v: Morlino, G, Blasi, P, Peretti, E & Cristofari, P 2021, ' Particle acceleration in winds of star clusters ', Monthly Notices of the Royal Astronomical Society, vol. 504, no. 4, pp. 6096-6105 . https://doi.org/10.1093/mnras/stab690
Monthly Notices of the Royal Astronomical Society (MNRAS)

The origin of cosmic rays in our Galaxy remains a subject of active debate. While supernova remnant shocks are often invoked as the sites of acceleration, it is now widely accepted that the difficulties of such sources in reaching PeV energies are da

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e297f3694ec21f119ef9d41ef56380e5
https://curis.ku.dk/portal/da/publications/particle-acceleration-in-winds-of-star-clusters(44435def-bd31-41ba-87b5-ff661fdea000).html

Particle acceleration and multimessenger emission from starburst-driven galactic winds

Autor: Pasquale Blasi, Markus Ahlers, Giovanni Morlino, Enrico Peretti

Publikováno v: Peretti, E, Morlino, G, Blasi, P & Cristofari, P 2022, ' Particle acceleration and multimessenger emission from starburst-driven galactic winds ', Monthly Notices of the Royal Astronomical Society, vol. 511, no. 1, pp. 1336-1348 . https://doi.org/10.1093/mnras/stac084

The enhanced star forming activity, typical of starburst galaxies, powers strong galactic winds expanding on kiloparsec (kpc) scales and characterized by bubble structures. Here we discuss the possibility that particle acceleration may take place at

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d542e8ad8f23ec19c6faf143b09175c4