Scheda Good OMENS
FINAL
Informazioni generali
Good Old Magnetism in the Early uNiverSe
Good OMENS
Programma
RSN1
Attività: Nuova; Data inizio: 2022; Data fine: 2030
daniela.paoletti daniela.paoletti@inaf.it
L’origine del magnetismo cosmico è uno dei puzzle ancora irrisolti della cosmologia moderna; la presenza di campi magnetici su scale cosmologiche richiede un contributo da campi seminali generati nell’Universo primordiale. Questi campi magnetici primordiali a loro volta influenzano l’intera storia dell’Universo lasciando impronte sul fondo cosmico a microonde (CMB) e la struttura su grande scala (LSS). Da 14 anni INAF è rinomato a livello internazionale nel campo dello studio dei campi magnetici primordiali e le loro sinergie con la CMB e LSS. I ricercatori intendono proseguire le attività in questo campo in preparazione per i futuri esperimenti che con la loro precisione permetteranno di risolvere il puzzle dell’origine del magnetismo cosmico.
The origin of cosmic magnetism is one of the still unsolved puzzle of modern cosmology; the presence of magnetic fields on cosmological scales requires a contribution from seed fields generated in the Early Universe. Such primordial magnetic fields in turn influence all the Universe history leaving imprints on the Cosmic Microwave Background radiation (CMB) and the Large Scale Structure (LSS). In the last 14 years INAF has been internationally renowned in the study of primordial magnetic fields and their synergies with CMB and LSS. The researchers want to continue the activities in this field in preparation for future experiments that with their precision will allow to solve the puzzle on the 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 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| OAS BOLOGNA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 1 | 0.15 |
| Totali | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 1 | 0.15 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 5
| # | Struttura | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | 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 2022 | Certi 2023 | Certi 2024 | Presunti 2022 | Presunti 2023 | Presunti 2024 |
|---|---|---|---|---|---|
| 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. 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; the Coordinator is also one of the developers of the first code to predict the heating effect on CMB anisotropies.</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;">The Coordinator has been the leader of the working group dedicated to Primordial Magnetic Fields in the Planck Collaboration 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"><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;">The Coordinator is currently the leader of the Project Study Group dedicated to Primordial Magnetic Fields in the LiteBIRD Collaboration.</span></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 (2022/2023/2024) | FTE Presunte (2022/2023/2024) | 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 (2022/2023/2024) | FTE Presunte (2022/2023/2024) | 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 TD | MHD Simulations | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
| 5 | franco.vazza | franco.vazza2@unibo.it | Università di Bologna | Y | Professore 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). Associato a questa scheda verrà richiesto un minigrant per finanziare visiting scientists sia in ingresso che in uscita e per meetings.
Tabella fondi:
| # | 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€) |
|---|
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2022 (€) | Fondi 2023 (€) | Fondi 2024 (€) |
|---|