首页|Radiation Spectral Analysis of 3D Dust Molecular Clusters(PAHs)and Peptoids under Ionization and Electric Field in ISM

Radiation Spectral Analysis of 3D Dust Molecular Clusters(PAHs)and Peptoids under Ionization and Electric Field in ISM

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Polycyclic aromatic hydrocarbons(PAHs),PANHs,and peptoids dust spectral calculations from the interstellar medium(ISM)are important for dust observations and theory.Our goal is to calculate the radiation spectrum of spherical PAHs dust clusters in a vacuum containing ionized and applied in the presence of an electric field.We propose a new simple computational model to calculate the size of three-dimensional spherical dust clusters formed by different initial dust structures.By the Vienna Ab-initio Simulation Package code,the density functional theory with the generalized approximation was used to calculate the electron density gradient and obtain the radiation spectrum of dust.When the radius of spherical dust clusters is~[0.009-0.042]μm,the dust radiation spectrum agrees well with the Z=0.02 mMMP stellar spectra,and the PAHs radiation spectrum of NGC 4676 at wavelengths of(0-5]μm and(5-10]μm,respectively.In the ionized state,the N-PAH,C10H9N,2(C4H 4)1+,and peptoids 4(CHON),(C8H10N2O5)1+ dust clusters at 3.3 μm,while the 2(C22H21N3O 2)1+,4(CHON)dust clusters at 5.2 μm have obvious peaks.There is a characteristic of part of PAHs and peptoids clusters radiation at the near-infrared wavelength of 2 μm.However,especially after applying an electric field to the dust,the emission spectrum of the dust increases significantly in the radiation wavelength range[3-10]μm.Consequently,the dust clusters of PAHs,PANHs,and peptoids of the radius size~[0.009-0.042]μm are likely to exist in the ISM.

ISM:structureISM:moleculesradiation mechanisms:general(ISM:)dustextinction

Ruiqing Wu、Chunhua Zhu、Guoliang Lü、Xiaojiao Zhang、Xizhen Lu、Jinlong Yu、Wujin Chen、Mengqiu Long

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School of Physics and Electronics,Central South University,Changsha 410083,China

School of Physical Science and Technology,Xinjiang University,Urumqi 830046,China

School of Microelectronics and Physics,Hunan University of Technology and Business,Changsha 410205,China

College of Mechanical and Electronic Engineering,Tarim University,Alar 843300,China

School of Medicine,Xinjiang Medical University,Urumqi 830011,China

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Independent Innovation Project for Postgraduates of Central South University国家自然科学基金project of Xinjiang

160171008U20312042021D01C075

2024

天文和天体物理学研究
中国科学院国家天文台

天文和天体物理学研究

CSTPCD
影响因子:0.406
ISSN:1674-4527
年,卷(期):2024.24(1)
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