Scheda Good OMENS
FINAL
Informazioni generali
Good Old Magnetism in the Early uNiverSe
Good OMENS
Programma
RSN1
RSN4
Attività: In Itinere; Data inizio: 2023; Data fine: 2033
daniela.paoletti daniela.paoletti@inaf.it
L’origine del magnetismo cosmico è una delle grandi questioni irrisolte della cosmologia e l'ipotesi di una possibile origine nell’Universo primordiale è sempre più favorita dai dati. L'esistenza di campi magnetici primordiali implicherebbe la prova inequivocabile di violazioni del modello standard della fisica fondamentale e ne rappresentebbe un formidabile probe. Da anni INAF è rinomato a livello internazionale nello studio dei campi magnetici primordiali, le loro sinergie con CMB e LSS e la loro connessione col magnetismo cosmico. La Good OMENS rappresenta le attività in questo campo in preparazione per i futuri esperimenti che con la loro precisione permetteranno nei prossimi 10 anni di sciogliere la questione sull'origine primordiale del magnetismo cosmico.
The origin of cosmic magnetism is one of the great unsolved questions of
cosmology and the hypothesis of a possible origin in the early Universe
is increasingly favored by the data. The existence of primordial
magnetic fields implies the unequivocal proof of violations of the
standard model of fundamental physics and represents a
formidable probe. For years INAF has been internationally renowned in the study of primordial magnetic fields and their
synergies with the CMB and LSS and connection with cosmic magnetism. The Good OMENS represents the
activities in this field in preparation for future experiments which,
with their precision, will allow over the next 10 years to resolve the
question of the primordial origin of cosmic magnetism.
Cosmologia teorica ed osservativa
Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 3
| Struttura | Nfte | N0 | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| OAS BOLOGNA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 2 | 0.25 |
| Totali | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 2 | 0.25 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 5
| # | Struttura | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | SISSA | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0.00 |
| 2 | The Institute of Mathematical Sciences (Chennai, India) | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0.00 |
| 3 | CINECA | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
| 4 | Università Padova | 0 | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 |
| 5 | Università di Bologna | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0.00 |
| Totali | 0.30 | 0.30 | 0.30 | 0.00 | 0.00 | 0.00 | 0.00 |
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
| Certi 2023 | Certi 2024 | Certi 2025 | Presunti 2023 | Presunti 2024 | Presunti 2025 |
|---|---|---|---|---|---|
| 0 | 0 | 0 | 0 | 0 | 0 |
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
Informazioni Pubbliche
<p><span style="font-size:11pt;font-family:Arial;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;" id="docs-internal-guid-23bd244d-7fff-5ccb-5b81-6043270b90b0">Cosmology; Early Universe; Cosmic Microwave Background radiation; Cosmological Model; Cosmological Parameters; Large Scale Structure of the Universe; </span></p>
<p dir="ltr" style="line-height:1.2;background-color:#ffffff;margin-top:12pt;margin-bottom:0pt;padding:0pt 0pt 12pt 0pt;" id="docs-internal-guid-00bcc17e-7fff-cbcf-2d68-e9179c0f2bd5" align="justify"><span style="font-size:11pt;font-family:Arial;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">INAF has played a crucial role since 2007 in the development of primordial magnetic fields theoretical treatments and predictions of cosmological observable and in the study of the interplay of primordial magnetic fields science with CMB and LSS data. <font color="#000000">The Coordinator is the author and the owner of one of the two existing Einstein Boltzmann codes for the predictions of magnetically induced CMB anisotropy spectra, the only one with the exact magnetic source terms and the only one accurate enough for future CMB experiments precision; the Coordinator is also one of the developers of the first code to predict the heating effect on CMB anisotropies and again the only one available with a sufficient precision to investigate all models of PMF.</font></span></p><p dir="ltr" style="line-height:1.2;background-color:#ffffff;margin-top:0pt;margin-bottom:0pt;padding:0pt 0pt 12pt 0pt;" align="justify"><span style="font-size:11pt;font-family:Arial;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;"><font color="#0000FF">The Coordinator has been the leader of the working group dedicated to Primordial Magnetic Fields in the Planck Collaboration</font> from 2013 to the publication of the dedicated paper in 2016 (whose the Coordinator is corresponding author): Planck 2015 results XIX:Constraints on Primordial Magnetic Fields.</span></p><p dir="ltr" style="line-height:1.2;background-color:#ffffff;margin-top:0pt;margin-bottom:12pt;" align="justify"><font color="#9C00FF"><span style="font-size: 11pt; font-family: Arial; background-color: transparent; font-weight: 400; font-style: normal; font-variant: normal; text-decoration: none; vertical-align: baseline; white-space: pre-wrap;">The Coordinator is currently the leader of the Project Study Group dedicated to Primordial Magnetic Fields in the LiteBIRD Collaboration.</span></font></p><p></p>
<p><span style="font-size:11.5pt;font-family:Arial;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;" id="docs-internal-guid-51c41fc4-7fff-7ce8-9a0c-69bbb0b52283">Planck; LiteBIRD; Simons Observatory; CMB-S4; Euclid; INAF-OAS cluster; CINECA</span><span style="font-size:10.5pt;font-family:Arial;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">.</span></p>
15. Team members, Informazioni generali
15. Personale INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | daniela.paoletti | daniela.paoletti@inaf.it | OAS BOLOGNA | N | RICERCATORE | Coordinatore | X X X | X X X | X |
|
| 2 | fabio.finelli | fabio.finelli@inaf.it | OAS BOLOGNA | Y | PRIMO RICERCATORE | Forecasts; | X X X | X X X | X |
|
| 3 | alessandro.gruppuso | alessandro.gruppuso@inaf.it | OAS BOLOGNA | Y | RICERCATORE | Interplay with the cosmological model | X X X | X X X | X |
|
16. Personale Associato INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | carlo.baccigalupi | carlo.baccigalupi@sissa.it | SISSA | Y | CMBXC SWG Coordinatore | Forecasts | [0.1, 0.1, 0.1] | [0.0, 0.0, 0.0] | 0.0 |
| 2 | dhiraj.hazra | dhiraj@imsc.res.in | The Institute of Mathematical Sciences (Chennai, India) | Y | Reader | Interplay with the cosmological model | [0.1, 0.1, 0.1] | [0.0, 0.0, 0.0] | 0.0 |
| 3 | diego.molinari | diego.molinari@inaf.it | CINECA | Y | User Support staff | Forecasts; Interplay with cosmological model | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
| 4 | elisa.prandini | elisa.prandini@unipd.it | Università Padova | N | Ricercatrice TDb | MHD Simulations | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
| 5 | franco.vazza | franco.vazza2@unibo.it | Università di Bologna | Y | Prof. Associato | MHD Simulations | [0.1, 0.1, 0.1] | [0.0, 0.0, 0.0] | 0.0 |
21. Fondi a Sostegno Iniziativa
Le attività di Good OMENS non hanno mai ricevuto finanziamenti dedicati, la PI è sempre stata supportata da fondi esterni dedicati ad altri progetti (Planck, ASI-Cosmos, LiteBIRD).
Tabella fondi:
| # | Provenienza | Certi 2023 (k€) | Certi 2024 (k€) | Certi 2025 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
|---|
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2023 (€) | Fondi 2024 (€) | Fondi 2025 (€) |
|---|