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Chen, Tao
Publications (8 of 8) Show all publications
Chen, T. & Luo, Y. (2019). Formation of polyynes and ring-polyyne molecules following fragmentation of polycyclic aromatic hydrocarbons. Monthly notices of the Royal Astronomical Society, 486(2), 1875-1881
Open this publication in new window or tab >>Formation of polyynes and ring-polyyne molecules following fragmentation of polycyclic aromatic hydrocarbons
2019 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 486, no 2, p. 1875-1881Article in journal (Refereed) Published
Abstract [en]

In this work, we perform molecular dynamic (MD) simulations to investigate the stability and fragmentation processes of vibrationally excited linear polycyclic aromatic hydrocarbons (PAHs). The program of CP2K in combination with the semi-empirical method PM3 is utilized for the MD simulations. The simulations show that the formation of molecular hydrogens (H-2) is different than previous studies, in particular, different than compact PAHs. At high temperatures, linear PAHs tend to open aromatic rings and convert the sp(3) C-C or sp(2) C=C bonds to sp C C bonds by removing H-2; i.e. polyynes are formed in such process. Besides polyynes, PAHs attached with sp-bonded polyyne chains are commonly observed at high temperatures. We notice that due to the addition of flexible tails (polyynes), the ring-polyyne molecules do not dissociate for a long period of time at high temperatures. Such structures facilitate the molecules to survive in the harsh environment of the interstellar medium. In addition, the ring-polyyne structures induce dipole moments that could, in principle, be detected by radio astronomy.

Place, publisher, year, edition, pages
OXFORD UNIV PRESS, 2019
Keywords
astrochemistry, molecular processes, methods: laboratory: molecular, ISM: molecules, photodissociation region (PDR)
National Category
Theoretical Chemistry
Identifiers
urn:nbn:se:kth:diva-255492 (URN)10.1093/mnras/stz1014 (DOI)000474899400033 ()2-s2.0-85067965367 (Scopus ID)
Note

QC 20190918

Available from: 2019-09-18 Created: 2019-09-18 Last updated: 2019-09-18Bibliographically approved
Zhang, W., Si, Y., Zhen, J., Chen, T., Linnartz, H. & Tielens, A. G. G. (2019). Laboratory Photochemistry of Covalently Bonded Fluorene Clusters: Observation of an Interesting PAH Bowl-forming Mechanism. Astrophysical Journal, 872(1), Article ID 38.
Open this publication in new window or tab >>Laboratory Photochemistry of Covalently Bonded Fluorene Clusters: Observation of an Interesting PAH Bowl-forming Mechanism
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2019 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 872, no 1, article id 38Article in journal (Refereed) Published
Abstract [en]

The fullerene C-60, one of the largest molecules identified in the interstellar medium (ISM), has been proposed to form top-down through the photochemical processing of large (more than 60 C atoms) polycyclic aromatic hydrocarbon (PAH) molecules. In this article, we focus on the opposite process, investigating the possibility that fullerenes form from small PAHs, in which bowl-forming plays a central role. We combine laboratory experiments and quantum chemical calculations to study the formation of larger PAHs from charged fluorene clusters. The experiments show that with visible laser irradiation, the fluorene dimer cation-[C13H9-C13H9](+)-and the fluorene trimer cation-[C13H9-C13H8-C13H9](+)-undergo photodehydrogenation and photoisomerization, resulting in bowl-structured aromatic cluster ions, C26H12+ and C39H20+, respectively. To study the details of this chemical process, we employ quantum chemistry that allows us to determine the structures of the newly formed cluster ions, to calculate the dissociation energies for hydrogen loss, and to derive the underlying reaction pathways. These results demonstrate that smaller PAH clusters (with less than 60 C atoms) can convert to larger bowled geometries that might act as building blocks for fullerenes, because the bowl-forming mechanism greatly facilitates the conversion from dehydrogenated PAHs to cages. Moreover, the bowl-forming induces a permanent dipole moment that-in principle-allows one to search for such species using radio astronomy.

Place, publisher, year, edition, pages
IOP PUBLISHING LTD, 2019
Keywords
astrochemistry, ISM: molecules, methods: laboratory: molecular, molecular processes ultraviolet, ISM
National Category
Chemical Sciences
Identifiers
urn:nbn:se:kth:diva-247839 (URN)10.3847/1538-4357/aafe10 (DOI)000460810800002 ()2-s2.0-85062022618 (Scopus ID)
Note

QC 20190326

Available from: 2019-03-26 Created: 2019-03-26 Last updated: 2019-04-04Bibliographically approved
Chen, T. (2019). Temperature effects on anharmonic infrared spectra of large compact polycyclic aromatic hydrocarbons. Astronomy and Astrophysics, 622, Article ID A152.
Open this publication in new window or tab >>Temperature effects on anharmonic infrared spectra of large compact polycyclic aromatic hydrocarbons
2019 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 622, article id A152Article in journal (Refereed) Published
Abstract [en]

Aims. Large compact polycyclic aromatic hydrocarbon molecules (PAHs) present special interest in the astrochemical community. A key issue in analyses of large PAHs is understanding the effect that temperature and anharmonicity have on different vibrational bands, and thus interpreting the infrared (IR) spectra for molecules under various conditions. Methods. Because of the huge amount of interactions/resonances in large PAHs, no anharmonic IR spectrum can be produced with static/time-independent ab initio method, especially for the molecules with D6h symmetry, e.g., coronene and circumcoronene. In this work, we performed molecular dynamics simulations to generate anharmonic IR spectra of coronene and circumcoronene. Results. The method is validated for small PAHs, i.e., naphthalene and pyrene. We find that the semiempirical method PM3 produces accurate band positions with an error <5 cm(-1). Furthermore, we calculate the spectra at multiple temperatures and find a clear trend toward band shifting and broadening.

Place, publisher, year, edition, pages
EDP SCIENCES S A, 2019
Keywords
astrochemistry, techniques: spectroscopic, line: profiles, molecular data, ISM: lines and bands, methods: laboratory: molecular
National Category
Theoretical Chemistry
Identifiers
urn:nbn:se:kth:diva-244507 (URN)10.1051/0004-6361/201834518 (DOI)000458360200001 ()2-s2.0-85061738025 (Scopus ID)
Note

QC 20190402

Available from: 2019-04-02 Created: 2019-04-02 Last updated: 2019-04-04Bibliographically approved
Chen, T., Mackie, C., Candian, A., Lee, T. J. & Tielens, A. G. G. (2018). Anharmonicity and the infrared emission spectrum of highly excited polycyclic aromatic hydrocarbons. Astronomy and Astrophysics, 618, Article ID A49.
Open this publication in new window or tab >>Anharmonicity and the infrared emission spectrum of highly excited polycyclic aromatic hydrocarbons
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2018 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 618, article id A49Article in journal (Refereed) Published
Abstract [en]

Aims. Infrared (IR) spectroscopy is a powerful tool to study molecules in space. A key issue in such analyses is understanding the effect that temperature and anharmonicity have on different vibrational bands, and thus interpreting the IR spectra for molecules under various conditions. Methods. We combined second order vibrational perturbation theory and the Wang-Landau random walk technique to produce accurate IR spectra of highly excited polycyclic aromatic hydrocarbons. We fully incorporated anharmonic effects, such as resonances, overtones, combination bands, and temperature effects. Results. The results are validated against experimental results for the pyrene molecule (C16H10). In terms of positions, widths, and relative intensities of the vibrational bands, our calculated spectra are in excellent agreement with gas-phase experimental data.

Place, publisher, year, edition, pages
EDP Sciences, 2018
Keywords
astrochemistry, ISM: lines and bands, photon-dominated region
National Category
Physical Sciences
Identifiers
urn:nbn:se:kth:diva-237092 (URN)10.1051/0004-6361/201833731 (DOI)000446951000006 ()
Note

QC 20181024

Available from: 2018-10-24 Created: 2018-10-24 Last updated: 2018-10-24Bibliographically approved
Chen, T. (2018). Formation of Covalently Bonded Polycyclic Aromatic Hydrocarbons in the Interstellar Medium. Astrophysical Journal, 866(113)
Open this publication in new window or tab >>Formation of Covalently Bonded Polycyclic Aromatic Hydrocarbons in the Interstellar Medium
2018 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 866, no 113Article in journal (Refereed) Published
Abstract [en]

Photo-/ion-induced ionization and dissociation processes are commonly observed for polycyclic aromatic hydrocarbon (PAH) molecules. This work performs theoretical studies of PAHs and their fragments. Molecular dynamics simulations in combination with static quantum chemical calculations reveal that following a single hydrogen atom loss, the fragments, PAH-H, are extremely reactive. They catch a neighbor molecule within picoseconds to form a covalently bonded large molecule regardless of orientations/angles and temperatures. We calculate the infrared spectra of the covalently bonded molecules, which indicate that such species could be the carrier of unidentified infrared emission bands. It also implies that regular PAHs might be less abundant in space than what is expected. 

Place, publisher, year, edition, pages
Institute of Physics (IOP), 2018
Keywords
astrochemistry; ISM: molecules; infrared: ISM; line: formation; methods: laboratory: molecular
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
urn:nbn:se:kth:diva-238817 (URN)10.3847/1538-4357/aae38f (DOI)000456434400012 ()2-s2.0-85055585545 (Scopus ID)
Note

QC 20181217

Available from: 2018-11-12 Created: 2018-11-12 Last updated: 2019-02-12Bibliographically approved
Zhen, J., Chen, T. & Tielens, A. G. G. (2018). Laboratory Photochemistry of Pyrene Clusters: An Efficient Way to Form Large PAHs. Astrophysical Journal, 863(2), Article ID 128.
Open this publication in new window or tab >>Laboratory Photochemistry of Pyrene Clusters: An Efficient Way to Form Large PAHs
2018 (English)In: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 863, no 2, article id 128Article in journal (Refereed) Published
Abstract [en]

In this work, we study the photodissociation processes of small PAH clusters (e.g., pyrene clusters). The experiments are carried out using a quadrupole ion trap in combination with time-of-flight (QIT-TOF) mass spectrometry. The results show that pyrene clusters are converted into larger PAHs under the influence of a strong radiation field. Specifically, pyrene dimer cations (e.g., [C16H10-C16H9](+) or C32H19 (+)), will photodehydrogenate and photo-isomerize to fully aromatic cations (PAHs) (e.g., C32H16 (+)) with laser irradiation. The structure of new formed PAHs and the dissociation energy for these reaction pathways are investigated with quantum chemical calculations. These studies provide a novel efficient evolution routes for the formation of large PAHs in the interstellar medium in a bottom-up process that will counteract the top-down conversion of large PAHs into rings and chains, and provide a reservoir of large PAHs that can be converted into C-60 and other fullerenes and large carbon cages.

Place, publisher, year, edition, pages
Institute of Physics Publishing (IOPP), 2018
Keywords
astrochemistry, ISM: molecules, methods: laboratory: molecular, molecular processes ultraviolet: ISM
National Category
Atom and Molecular Physics and Optics
Identifiers
urn:nbn:se:kth:diva-234609 (URN)10.3847/1538-4357/aad240 (DOI)000442070500005 ()2-s2.0-85052402058 (Scopus ID)
Note

QC 20180914

Available from: 2018-09-14 Created: 2018-09-14 Last updated: 2018-09-14Bibliographically approved
Chen, T. (2018). The Carrier of 3.3 mu m Aromatic Infrared Bands: Anharmonicity and Temperature Effects on Neutral PAHs. Astrophysical Journal Supplement Series, 238(2), Article ID 18.
Open this publication in new window or tab >>The Carrier of 3.3 mu m Aromatic Infrared Bands: Anharmonicity and Temperature Effects on Neutral PAHs
2018 (English)In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 238, no 2, article id 18Article in journal (Refereed) Published
Abstract [en]

Anharmonic infrared (IR) spectra are crucial for the study of interstellar polycyclic aromatic hydrocarbon (PAH) molecules. This work aims to provide a comprehensive study of the features that may influence the accuracy of anharmonic IR spectra of PAHs so that a reliable spectrum that incorporates all necessary features for interpreting the observational IR spectra can be obtained. Six PAHs are investigated: naphthalene, anthracene, pyrene, chrysene, 9,10-dimethylanthracene, and 9,10-dihydroanthracene. The NIST spectra and high-resolution IR absorption spectra are utilized as the reference for the comparisons. The influences of different resonances and resonant thresholds are studied. Four methods for electronic structure calculations are tested. The quantitative comparisons indicate that for the NIST data, B3LYP/NO7D provides the best agreement with measured spectra concerning band positions and B3LYP/cc-pVTZ is superior in the description of the relative intensities. The importance of 1-3 Darling-Dennison resonances, which are required for generating triple combination bands, is investigated through a comparison to a high-resolution experimental spectrum. For interpreting the bandwidths and profiles of the observational spectra, the temperature effects are included through the Wand-Landau random walk technique. The comparisons between calculated high-temperature anharmonic and observational spectra indicate that small and compact PAHs might be responsible for the 3.3 mu m aromatic infrared bands.

Place, publisher, year, edition, pages
Institute of Physics Publishing (IOPP), 2018
Keywords
astrochemistry, infrared: ISM, ISM: molecules, line: identification, line: profiles, techniques: spectroscopic
National Category
Physical Sciences
Identifiers
urn:nbn:se:kth:diva-237117 (URN)10.3847/1538-4365/aadcae (DOI)000446184800001 ()2-s2.0-85055708273 (Scopus ID)
Funder
Swedish Research Council, 2015-06501Swedish National Infrastructure for Computing (SNIC), SNIC 2018/3-30
Note

QC 20180930

Available from: 2018-10-30 Created: 2018-10-30 Last updated: 2019-05-07Bibliographically approved
Chen, T., Zhen, J., Wang, Y., Linnartz, H. & Tielens, A. G. (2017). Photodissociation processes of Bisanthenquinone cation. Proceedings of the International Astronomical Union (S332), 353-359
Open this publication in new window or tab >>Photodissociation processes of Bisanthenquinone cation
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2017 (English)In: Proceedings of the International Astronomical Union, ISSN 1743-9213, no S332, p. 353-359Article in journal (Refereed) Published
Abstract [en]

A systematic study, using ion trap time-of-flight mass spectrometry, is presented for the photo-dissociation processes of Bisanthenquinone (Bq) cations, C28H12O2+, a ketone substituted Polycyclic Aromatic Hydrocarbon (PAH). The Bq cation fragments through sequential loss of the two neutral carbonyl (CO) units upon laser (626nm) irradiation, resulting in a PAH-like derivative C26H12+. Upon further irradiation, C26H12+ exhibits both stepwise dehydrogenation and C2/C2H2 loss fragmentation channels. Quantum chemistry calculations reveal a detailed picture for the first CO-loss, which involves a transition state with a barrier of ∼ 3.4 eV, which is lower than the energy required for the lowest H-loss pathway (∼ 5.0 eV). The barrier for the second CO-loss is higher (∼ 4.9 eV). The subsequent loss of this unit changes the Bq geometry from a planar to a bent one. It is concluded that the photodissociation mechanism of the substituted PAH cations studied here is site selective in the substituted subunit. This work also shows that an acetone substituted PAH cation is not photo-stable upon irradiation. 

Place, publisher, year, edition, pages
Cambridge University Press, 2017
Keywords
carbonyl, molecule, PAH, photodissociation, quinone, TOF
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
urn:nbn:se:kth:diva-236844 (URN)10.1017/S1743921317007864 (DOI)2-s2.0-85052742768 (Scopus ID)
Note

QC 20181220

Available from: 2018-12-20 Created: 2018-12-20 Last updated: 2019-08-27Bibliographically approved
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