Laboratory Simulation of the Positron-Dust Interaction and its Implication for Interstellar Dark Clouds
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389021%3A_____%2F23%3A00573218" target="_blank" >RIV/61389021:_____/23:00573218 - isvavai.cz</a>
Alternative codes found
RIV/68378271:_____/23:00567741 RIV/00216208:11320/23:10469102 RIV/68407700:21460/23:00363276 RIV/68407700:21670/23:00363276
Result on the web
<a href="https://iopscience.iop.org/article/10.3847/1538-4357/aca01c" target="_blank" >https://iopscience.iop.org/article/10.3847/1538-4357/aca01c</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/aca01c" target="_blank" >10.3847/1538-4357/aca01c</a>
Alternative languages
Result language
angličtina
Original language name
Laboratory Simulation of the Positron-Dust Interaction and its Implication for Interstellar Dark Clouds
Original language description
We report the first laboratory experiment dealing with the interaction of a cosmic dust simulant with positrons emitted from a 22Na radioisotope. Measurements of a charge of micrometer SiO2 dust grains with an accuracy of one elementary charge e revealed +1 e steps due to positron annihilation inside the grain. The observed average rate of these charging events agrees well with prediction of a model based on the continuous slowing down approximation of energetic of positrons inside the grain. Less frequent charge steps larger than +1 e were attributed to emission of secondary electrons during positron slowing down. The determined coefficient of secondary electron emission is approximately inversely proportional to the grain radius. The experimental results led us to the formulation of a possible scenario of interstellar dark clouds charging.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10305 - Fluids and plasma physics (including surface physics)
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal
ISSN
0004-637X
e-ISSN
1538-4357
Volume of the periodical
942
Issue of the periodical within the volume
1
Country of publishing house
GB - UNITED KINGDOM
Number of pages
13
Pages from-to
42
UT code for WoS article
000908109100001
EID of the result in the Scopus database
2-s2.0-85146166671