ASTRONOMY WITH RADIOACTIVITIES
SEP 29 - OCT 02, 1999
INTERNATIONAL WORKSHOP
AT THE RINGBERG
CASTLE
OF THE
MAX PLANCK GESELLSCHAFT
KREUTH, TEGERNSEE, GERMANY
and more information on:
Scope:
Astronomy with radioactivities as a subfield of nuclear astrophysics addresses
the astrophysical potential of measurements of cosmic radioactive isotopes.
Since the first detection of a cosmic radioactivity line back in the 60ies,
almost 30 years of hard experimental effort has helped to advance this
field into an astronomical regime of its own: Gamma-rays transmit radioactive
decay to the observer most directly, and radioisotopes are most direct
messengers from the nuclear processes in stellar interiors and explosive
environments. But radioactivities also encode cosmic-ray history between
sources and observations in near-earth space, and solar-system meteorites
have been found to include traces of radioactive decay in grains which
must have formed close to nucleosynthesis sites.
Experimental techniques of today can image the sky in radioactivity
gamma-rays to a precision sufficient to perform correlation studies with
other astronomical sources. Even the radioactive motors of supernovae are
at the rim of measurement capabilities through decay gamma-rays from shortlived
Ni and Co. Charged-particle detectors capture and analyze isotopic distributions
in regions of the solar system which are remote from the earth magnetic
field distortions, and precision isotopic analyses in laboratories of meteoritic
grains down to microns in diameter has established a rich body of astronomical
data. Supplementing these astronomical enterprises, radioactive-beam facilities
are beginning to provide support for nuclear-reaction cross sections in
previously unexplored regimes. Furthermore, the evolution of computing
facilities makes even multi-dimensional hydrodynamical modeling of stars
and explorion with coupled large nuclear-reaction networks a feasible perspective,
thus helping our interpretation and models of cosmic radioactivities.
With this workshop, we aim to expose the context of astronomical studies
with radioactivities along above aspects. The roots of the workshop are
COMPTEL Team-internal small workshops centered on 26Al imaging
in gamma-rays, and the science workshop "The Radioactive Galaxy" held at
Clemson University in March 1996.
Contents
The workshop started mid-day on Wednesday, September 29, and ended mid-day
Saturday, October 02, 1999.
The workshop took up the issues resulting from our previous workshops::
-
how do massive stars fill the ISM with longlived
26Al
and positrons?
-
how is 44Ti produced, so we see only so
few sources?
-
what can we conclude for the physical conditions
in those sources?
Naturally this led us, in addition to exposing the sources and the gamma-ray
data with their constraints, to add a closer look at the early SNR
phase, including acceleration of cosmic rays, and to discuss the possibility
of dust carrying some of the radioactive ejecta. The latter implied
that we discussed meteoritic isotopic anomalies, cosmic ray composition,
and why the solar nebula has some remarkable anomalies in radioactivity
traces.
The "sessions" of the workshop featured introductory/overview talks
and more specific contributed talks.
Program
-
Production of Radioisotopes in Stars (massive&AGB),
Supernovae, Novae, and the ISM
Nuclear reactions and networks, hydrodynamic models of stellar interiors
and explosions, and cosmic-ray spallation physics
(Speakers: Arnould, Meynet, Langer, Gallino, Mowlavi, Thielemann,
Hillebrandt, Hernanz, Woosley, Kifonidis)
-
Propagation and Fate of Radioisotopes in their
Source Vicinity
Early SNR phases with initial molecule and dust formation, WR winds,
nova envelopes, dust processing in ISM, acceleration of cosmic rays
(Speakers: Chevalier, Clayton, Woitke, Ramaty, Montmerle, Ellison)
-
Radioisotope Decay Gamma-Rays
26Al and 60Fe diffuse emission, supernova and
nova disgnostics in shortlived (<100y) radioactivity lines (44Ti,
56Ni,
22Na)
(Speakers: Knödlseder, Oberlack, Iyudin, The, Kumagai)
-
Annihilation and its Gamma-Rays
511 keV emission from galactic disk and sources, positron sources in
the galaxy (compact objects versus diffuse radioactivity)
(Speakers: Milne)
-
Presolar Meteoritic Radioactivity Studies
Presolar grain analysis from meteoritic inclusions, their implications
for dust formation and nucleosynthesis environments in AGB stars and SNae
(Speakers: Amari, Hoppe)
-
Isotopes in the Solar System
Cosmic-ray nuclear reactions in early solar nebula and present solar
system, direct isotope measurements through space probes and meteoritic
analyses
(Speakers: Meyer, Lugmair, DuVernois)
-
Radioisotopes and Evolution of Protostellar Systems,
Associations, and the Galaxy
Cosmochronometers, abundance and star formation budget & histories,
their relation to Galactic evolution
(Speakers: Montmerle, Prantzos, Truran, Faestermann, Korschinek,
Hartmann, Plüschke)
-
Astronomical Capabilities and Opportunities
Perspectives for cosmic radioactivity measurements: gamma-ray telescopes,
cosmic-ray composition explorers, presolar-grain isotopic analyses
(Speakers: von Ballmoos, Kurfess, Aprile)
Talks were 25 minutes, discussion followed as required.
Opportunities for discussions were a main workshop goal, through
extended breaks and during a hiking session in the local mountains, as
well as a special discussion evening.
Organisation
The workshop organisation was informal and low-cost. No conference fees.
Scientific organisation team members are
- Roland Diehl (MPE, also Contact Person / Coordinator, rod@mpe.mpg.de),
- Dieter Hartmann (Clemson)
- Mark Leising (Clemson)
- Nikos Prantzos (IAP).
The workshop location was the Ringberg
Castle of the Max Planck Gesellschaft, located approximately a one-hour
drive southeast of Munich, Germany. Full-board lodging at the castle was
available for participants, approximate cost 70 Euro/day.
Participation was by invitation and upon request to the organizing
team. The total number of participants was limited to approximately 60.
All workshop information is published on this website.
Proceedings
The Workshop Proceedinga are published as a booklet ("MPE-Report")
holding at least "extended abstracts" (~2 pages) or full papers, as preferred,
for each contribution, for distribution among participants and interested
colleagues. Contributions were collected a few weeks after the workshop.
Distribution of Proceedings
in March 2000.
Reference:
Astronomy with Radioactivities, Eds. Roland
Diehl & Dieter Hartmann,
MPE Report 274, ISBN 0178-0719
The individual contributions may be obtained
in electronic form here.
See also Diehl R., Hartmann D. (2000):
"Astronomy with Radioactivities" Conference Summary, PASP, Vol. 112,
775, 1278
by rod@mpe.mpg.de
History
- 26Feb99: first announcement, scope & program
outline
- 22Apr99: add list of contributions
- 07Jun99: update text & program outline&participants
list
- 02Jul99: add detailed program, rearrange top links
- 29Jul99: revise dates, include second circular
- 22Nov99: add proceedings details
- 15Jan00: update for post-workshop use
- 25 May 2000: update after proceedings distribution;
link to other sites
- 08 Dec 2000: make exclusive for 1999 workshop