Published June 2017
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Possible explanation for the "Dark Matter X-ray line" at ∼3.5 keV by charge exchange between S16+ and neutrals
Creators
- 1. Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg (Germany)
- 2. IOQ, Friedrich-Schiller-Universität, Max-Wien-Platz 1, 07743 Jena (Germany)
- 3. SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht (Netherlands)
- 4. Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden (Netherlands)
Description
Speculations about a possible dark matter origin of a weak x-ray transition at∼ 3.5keV have attracted enormous attention in the scientific community and given rise to a tide of publications attempting to explain the possible cause for this unidentified line-like feature.
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Additional details
Identifiers
Publishing Information
- Imprint Title
- Atomic Processes in Plasmas. Summary Report of Joint ICTP-IAEA School
- Imprint Pagination
- 76 p.
- Journal Page Range
- p. 35
- Report number
- INDC(NDS)--0723
Conference
- Title
- Joint ICTP-IAEA School on Atomic Processes in Plasmas
- Dates
- 27 Feb - 3 Mar 2017
- Place
- Trieste (Italy)
INIS
- Country of Publication
- International Atomic Energy Agency (IAEA)
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 50008609
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHARGE EXCHANGE; KEV RANGE 01-10; NONLUMINOUS MATTER; X RADIATION
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; ENERGY RANGE; IONIZING RADIATIONS; KEV RANGE; MATTER; RADIATIONS
Optional Information
- Notes
- 1 fig.