CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS

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CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
This project has received funding from
             the European Union’s Horizon 2020
             research and innovation programme
             under grant agreement No 101008324
             (ChETEC-INFRA).

ChETEC – INFRA
Chemical Elements as Tracers
of the Evolution of the Cosmos
- Infrastructures for nuclear
astrophysics

Tuesday 04.05.2021, 09:40 – 10:00

Daniel Bemmerer               HZDR Dresden, DE
CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
Nuclear astrophysics at the intersection of three disciplines
                                                                                       GW170817 and its kilonova
                                                                                       E. Pian et al. (2017)
         Astrophysics
                                                                                                                                         co
                                                                                37.5
                                                                                                   1.5 d                         3.5 d   sy
                                                                                                                                         th

                                                                                 37                                                      (fo
  Astro-           Nuclear                                                                                                               ch
  nomy             Physics                                                                                                               0.0

                                                log[Luminosity (erg s–1 Å–1)]
                                                                                36.5                                                     su
                                                                                                                                         fro
                                                                                                                                         eje
                                                                                 36
                                                                                                                                         lat
                                                                                                   5.5 d                         6.5 d   ob
                                                                                37.5
                                                                                                                                         th
                                                                                                                                         of
                                                                                 37                                                      th

                                                                                                                                         wa
                                                                                36.5
                                                                                                                                         aft
                                                                                                                                         GW
                                                                                 36
                                                                                                                                         X-
                                                                                         10,000   20,000               10,000   20,000   wi
                                                                                                      Wavelength (Å)                     0.3
                                                                                                                                         fro
                                          Figure 3 | Kilonova models compared with the AT 2017gfo spectra.
                                          X-shooter spectra (black line) at the first four epochs and kilonova models:
                                                                                                                                         for
               NASA/Swift                                                                                                                jet
                                          dynamical ejecta (Ye = 0.1–0.4, orange), wind region with proton fraction
 04.05.2021   Daniel Bemmerer: ChETEC-INFRA
                                          Ye = 0.3 (blue) and Ye = 0.25 (green). The red curve represents the sum of                     wi
                                          the three model components.                                                                    an
CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
Nuclear astrophysics at the intersection of three disciplines
Counts / 0.05 MeV

                    107               E p = 156.2 keV, add-back          107              E p = 189.5 keV, add-back      107               E
                                             Signal                                              Signal
                    106                      Background (rescaled)       106                Orange:     Observations
                                                                                                 Background (rescaled)   106
                                                                                            for 17 globular
                         5                                                    5
                    10                 22Ne(p,γ)23Na                     10                 clusters                     105

                    104                                                  104                                             104

                    103                                                  103                                             103

                    102                                                  102                                             102
                                                   Singles sum, gated                              Singles sum, gated

                    10
                                                        Exp., bg. sub.
                                                                         10
                                                                                                  +0.3
                                                                                                     Exp., bg. sub.
                                                                                                                            10
                                                        Simulation
                                                                                           AGB star models,
                                                                                                     Simulation

                         0   2   4      6     8   10 12 14 16 18              0   2   4   6with
                                                                                             8 old
                                                                                                10 /12
                                                                                                     new14 22   16Ne(p,γ)
                                                                                                                    18    23Na0 rate
                                                                                                                                 2     4   6
                                                   F. Ferraro et al. (2018)                  E γ [MeV]

                             Astrophysics
                                                                                            A. Slemer et al. (2017)

          Astro-                            Nuclear
          nomy                              Physics

                         04.05.2021         Daniel Bemmerer: ChETEC-INFRA
CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
Nuclear astrophysics as an emerging field in Europe
u    COST Action ChETEC
     Chemical Elements as Tracers of the Evolution of the Cosmos
     30 European countries represented
     April 2017 – October 2021
     Forerunner of ChETEC-INFRA

u    Nuclear Physics in Astrophysics Conference series, since 2002
     Sponsored by the Nuclear Physics Division of the European Physical Society
     200+ participants
     2019 Mainz / Germany
     next: CERN Geneva
     Partner with ChETEC-INFRA to support NPA conference schools

u    Nuclei in the Cosmos conference series, every even year since 1990
     International conference alternates between Europe and non-European countries
     200+ participants
     2021 (!!) Chengdu / China

    04.05.2021   Daniel Bemmerer: ChETEC-INFRA
CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
ChETEC-INFRA, an EU-supported Starting Community of
Research Infrastructures for Nuclear Astrophysics

                     5.0 M€ EU HORIZON2020 support (2021-2025)

         TNA                            JRA                            NA
  Transnational Access        Joint Research Activities        Networking Activities
Infrastructure access        Infrastructure usability     Infrastructure networking
• 8 nuclear labs             • Targets                    • Complementary
• 4 telescopes               • Abundance corrections          Expermiments.
• 1 computer                 • Analysis pipelines         • Solar fusion+model
                                                          • Geochemistry/Astrophysics
                                                          • Outreach
       32 partners, 17 countries, largest EU project for nuclear astrophysics yet

 04.05.2021   Daniel Bemmerer: ChETEC-INFRA
CHETEC - INFRA - HIFIS AND HELMHOLTZ EVENTS
First pillar: TA Transnational Access to Research Infrastructures

8 nuclear labs: 3763 hours access
u  Charged particle beams
u  Neutron beams
u  Underground lab                             Any scientist from EU+associated
u  γ-process                                   countries may apply with their
u  Accelerator mass spectrometry               experiment / observation /
                                               computation ideas, no need to be
4 telescopes: 172 nights access                member of ChETEC-INFRA!
u   NOT Nordic Optical Telescope La Palma/ES
u   3 medium-sized telescopes in BG, CZ, LT
                                               Detailed information, including
                                               presentations of all facilities,
1 supercomputer: 8 million cpu hours access    today in the 11:30-13:00 and
u  Hull/UK viper cluster                       14:00-15:30 sessions.

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
Second pillar: JRA Joint Research Activities

JRA1 Astronuclear Lab
u  Targets
u  Detectors
u  Accelerator Mass Spectrometry

JRA2 Astronuclear HPC (high power              Any scientist may join and
computing)                                     contribute!
u  Tools for Access to HPC
u  Software Pipeline
                                               Breakout sessions tomorrow
u  Nucleosynthesis Codes                       09:30 – 11:00.

JRA3 Astronuclear Abundances
u  Database of Abundance Corrections           Presentation of the JRAs to the
u  Open-Source Stellar Pipeline                plenum tomorrow, in the
                                               11:30-12:45 session.

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
Third pillar: NA Networking Activities

NA1 Comprehensive Nuclear Astrophysics
u  Cross-collaboration
u  Galactic chemical evolution                   Networking results and tools will
                                                 be made available on the web, for
NA2 Dissemination, Outreach, Innovation
                                                 all scientists.
u  Masterclasses and Scientific Schools
u  Conference Outreach, Research-Industry Days

NA3 Astronuclear Library                         Breakout sessions tomorrow
                                                 09:30 – 11:00.
u  “Big Three” and solar fusion
u  Rate library, data, and metadata format

NA4 Mass Spectrometry Network                    Presentation of the NAs to the
                                                 plenum tomorrow, in the
u  Bridge to planetary science
                                                 13:45-15:30 session.

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
ChETEC-INFRA, 32 partners in 17 countries

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
Cross-cutting goals
Educate the next generation of scientists
u Start with high school students
u SNAQs for PhD students already started !, reach+activate several 100 partipants

Increase participation across Europe+, across genders, nationalities, …
u  Conference outreach, web page, …
u  Top-level Gender and Inclusiveness Coordinator

Synergies and coherence with neighboring communities
u Large telescopes, labs, and supercomputers
u Links between astro and planetary sciences
u Links to US IRENA, China, Japan, …
u Links to COST actions ChETEC, GAIA-MW, PHAROS, ...

Interdisciplinary approaches
u  TNA proposals using more than one type of infrastructure are encouraged
u  Education of one PhD student in all three disciplines (observation, nuclear, astro)

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
ChETEC-INFRA, takeaway messages
Basic facts
u 32 partners in 17 EU+ countries
u ChETEC-INFRA runs 01 May 2021 – 30 April 2025
u 5.0 M€ support from EU research infrastructure networking budget
u We are a starting community, meaning we are meant to learn

What does it already mean for you?
u Network of research infrastructures to serve nuclear astrophysics
u ChETEC-INFRA access to research infrastructures is open to all
  scientists in EU+ countries, selection based on scientific merit

  04.05.2021   Daniel Bemmerer: ChETEC-INFRA
Structure of this kick-off meeting

Session             Topic
Tue 09:30-11:00     Welcome, COST actions, role model infrastructure networks, etc.
Tue 11:00           Conference photo
Tue 11:30-13:00     Transnational access (1)
Tue 14:00-15:30     Transnational access (2)
Tue 16:00-17:30     Closed session of General Assembly, votes (1 member per partner)

Wed 09:30-11:00     Breakout sessions for JRA and NA work packages
Wed 11:30-12:45     Presentations of JRA work packages
Wed 13:45-15:30     Presentations of NA work packages
Wed 16:00-17:30     International partners, and practical questions

 04.05.2021   Daniel Bemmerer: ChETEC-INFRA
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