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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • 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