Logo PUC-Rio Logo Maxwell
ETDs @PUC-Rio
Estatística
Título: PULSED LASER ABLATION OF IRON AND NICKEL TARGETS IN WATER AND ITS IMPLICATIONS IN ASTROCHEMISTRY
Autor: JOAO GABRIEL GIESBRECHT F PAIVA
Colaborador(es): TOMMASO DEL ROSSO - Orientador
DANIELE FULVIO - Coorientador
Catalogação: 02/DEZ/2021 Língua(s): ENGLISH - UNITED STATES
Tipo: TEXT Subtipo: THESIS
Notas: [pt] Todos os dados constantes dos documentos são de inteira responsabilidade de seus autores. Os dados utilizados nas descrições dos documentos estão em conformidade com os sistemas da administração da PUC-Rio.
[en] All data contained in the documents are the sole responsibility of the authors. The data used in the descriptions of the documents are in conformity with the systems of the administration of PUC-Rio.
Referência(s): [pt] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=56359&idi=1
[en] https://www.maxwell.vrac.puc-rio.br/projetosEspeciais/ETDs/consultas/conteudo.php?strSecao=resultado&nrSeq=56359&idi=2
DOI: https://doi.org/10.17771/PUCRio.acad.56359
Resumo:
The proposed research points to the possibility to perform CO2 reduction reaction (CO2RR) to solid carbon nanomaterials by the pulsed laser ablation (PLA) of magnetic target of iron (Fe) and nickel (Ni) in pure deionized water. The synthesized colloidal dispersions were characterized by different optical spectroscopies (UV-Vis, ICP-MS, FTIR and Raman) and transmission electron microscopy (TEM), revealing the presence of nanosized transition metal oxide and hydroxide nanoparticles, together with organic nanomaterial. The latter is well visible by TEM, energy-dispersive X-Ray spectroscopy (EDS), electron energy-loss spectroscopy(EELS), and Raman spectroscopy, which indicates the presence of amorphous graphitic carbon and CH vibrations. In the case of Ni derived nanomaterial, FTIR results confirm the presence of a beta-Ni(OH)2 hydroxide phase, while Raman and TEM measurements suggest also the presence of Ni(HCO3)2 nanosheets. The experimental results were finally discussed in the frame of the origin and evolution of simple and complex molecules of astrochemical interest, with special focus on those species potentially formed on the surface of metallic minor bodies in the solar system and cosmic dust grains in the interstellar medium(ISM).
Descrição: Arquivo:   
COMPLETE PDF