Theory Grant: "PEACE: Probing Extreme Acceleration in Cosmic Environment"
PEACE
Progetto
Programma
RSN4
Attività: Nuova; Data inizio: 2022; Data fine: 2024
martina.cardillo martina.cardillo@inaf.it
Cosmic particle acceleration is one of the most debated topics in High-Energy Astrophysics, largely studied through gamma-ray and neutrino emissions. The huge amount of data collected raised new questions on their nature and on the acceleration mechanisms at the basis of such extremely energetic radiation. Supernova Remnants, Pulsar Wind Nebulae, Microquasars, Blazars, AGN/starburst systems, despite having different nature, exhibit some surprising common aspects as sites of efficient particle acceleration. With theoretical models and a steady comparison with present and future data, we will carry on a parallel study of these different objects, to better understand how particle acceleration mechanisms translate into such a wide variety of phenomenological and spectral features.
Fisica degli oggetti compatti galattici ed extragalattici
Fenomeni non termici, raggi cosmici e astroparticelle
Struttura | Nfte | N0 | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Nex | Extra |
---|---|---|---|---|---|---|---|---|---|---|
IAPS ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
O.A. ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
Totali | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
Certi 2022 | Certi 2023 | Certi 2024 | Presunti 2022 | Presunti 2023 | Presunti 2024 |
---|---|---|---|---|---|
0.0 | 0.0 | 0.0 | 50.0 | 0.0 | 0.0 |
<p>High Energy Astrophysics; Gamma-rays; Gamma-ray sources; Plasma Astrophysics; Magnetic recconnection; Cosmi Ray sources; Galactic Cosmic Rays; CRAB Nebula; Pulsar Wind Nebulae; Supernova Remnants; Blazars; Jets; Active Galactic Nuclei; Neutrino Astronomy; Shock: Starburst Galaxies</p><p>Le linee di ricerca sono connesse a quelle di <span style="font-family: var(--bs-font-sans-serif); font-size: 1rem;">AGILE; ASTRI; MAGIC; CTA; CTA-LST; FERMI e delle seguenti schede INAF: scheda AGILE (Pittori), scheda PROGRESS (Antonelli), </span>scheda GAMMA2 (Vercellone); scheda Blazar (Vittorini); scheda CRAB (Vittorini); scheda Plasmi (Vittorini); scheda SSDC (Matteo Perri)</p><p><br></p>
<p class="MsoNormal" style="margin-top:12.0pt;margin-right:0cm;margin-bottom: 12.0pt;margin-left:0cm;text-align:justify;line-height:normal"><font color="#000000">According to <b>The INAF Strategic Vision documen</b>t (2019), <b>PEACE will support</b> the INAF research line followed in its large experimental programmes represented by the current g-ray facilities (e.g. <b>AGILE, MAGIC, LST1</b>) and forthcoming observatories (as <b>LST, ASTRI Mini-Array and CTA</b>), which play a crucial role in investigating the nature of PA and the origin of CRs. Even the <b>IXPE</b> telescope will pursue the study of polarization from cosmic accelerators to understand turbulence behaviour at the shock. In September 2022, the <b>INAF-OAR</b> will organize a <b>workshop</b> focused on PA with invited speakers and wide <b>round tables</b> about the state of the art of this topic. Part of our team is in LOC and SOC. The deep understanding and usage of ZELTRON code can also be related to other fields of interest for INAF, such as Solar physics. In the future, we may also contribute to projects like <b>SUNDISH</b>, devoted to space weather predictions, or <b>IXPE</b> in the polarization study of solar flares. </font><br></p>
<p>ASTRI; CTA; LST; MAGIC; SSDC</p>
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra | ||
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1 | martina.cardillo | martina.cardillo@inaf.it | IAPS ROMA | Y | RICERCATORE | Coordinator | X X X | X X X | X |
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2 | valerio.vittorini | valerio.vittorini@inaf.it | IAPS ROMA | Y | RICERCATORE | Member | X X X | X X X | X |
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3 | giovanni.piano | giovanni.piano@inaf.it | IAPS ROMA | Y | RICERCATORE | Member | X X X | X X X | X |
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4 | luca.foffano | luca.foffano@inaf.it | IAPS ROMA | N | ASSEGNISTA | Member | X X X | X X X | X |
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5 | eloisa.menegoni | eloisa.menegoni@inaf.it | IAPS ROMA | N | ASSEGNISTA | Member | X X X | X X X | X |
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6 | alessandra.lamastra | alessandra.lamastra@inaf.it | O.A. ROMA | Y | RICERCATORE | Member | X X X | X X X | X |
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7 | francesco.saturni | francesco.saturni@inaf.it | O.A. ROMA | N | ASSEGNISTA | Member | X X X | X X X | X |
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# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra |
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Possibili finanziamenti da parte di INAF (bando PRIN)
# | Provenienza | Certi 2022 (k€) | Certi 2023 (k€) | Certi 2024 (k€) | Presun. 2022 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
---|---|---|---|---|---|---|---|---|---|
1 | INAF | 0 | 0 | 0 | 50 | 0 | 0 | 0 | 50 |
# | Provenienza | Fondi 2022 (€) | Fondi 2023 (€) | Fondi 2024 (€) |
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