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20112023
most citedMagnetic Moment and Band Structure Analysis of Fe, Co, Ni-modified Graphene-nano- ribbon

3 citations · 18 across the 35 of their papers we have counts for

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Showing astro-ph.GAShow all

15 papers · 1 filter

astro-ph.GA2023

Classifying Protoplanetary disks Infrared Spectrum and Analysis by c-CH CH CH CH CH and CH to be Capable Template for Biological Molecule

Norio Ota, Aigen Li

Protoplanetary disk around a just born young star contains a lot of cosmic dust. especially polycyclic-aromatic-hydrocarbon (PAH), which would become basic component to create biol…

astro-ph.GA2021★ 2 cited

Magnetism of Fullerene C60 Compared with Graphene Molecule by DFT Calculation, Laboratory Experiment and Astronomical Observation

Norio Ota, Aigen Li, Laszlo Nemes +1

Magnetism of fullerene C60 was studied by three methods of the density functional theory (DFT) calculation, laboratory experiment and astronomical observation. DFT revealed that th…

astro-ph.GA2021

Void defect induced magnetism and structure change of carbon material-2, Graphene molecules

Norio Ota, Aigen Li, Laszlo Nemes +1

Void-defect is a possible origin of ferromagnetic feature on pure carbon materials. In our previous paper, void-defect on graphene-nanoribbon show highly polarized spin configurati…

astro-ph.GA2021

Void defect induced magnetism and structure change of carbon material-3, Polycyclic aromatic hydrocarbon

Norio Ota, Aigen Li, Laszlo Nemes

Void-defect induced magnetism of graphene molecule was recently reported in our previous paper of this series study. This paper investigated the case of hydrogenated graphene molec…

astro-ph.GA2020★ 1 cited

Graphene Molecules Contributing to the Infrared Bands of Carbon Rich Planetary Nebulae

Norio Ota, Aigen Li, Laszlo Nemes +1

It is well known since 2010 that fullerene C60 is widespread through the interstellar space. Also, it is well known that graphene is a source material for synthesizing fullerene. H…

astro-ph.GA2019★ 1 cited

Graphene Molecule Compared With Fullerene C60 As Circumstellar Carbon Dust Of Planetary Nebula

Norio Ota

It had been understood that astronomically observed infrared spectrum of carbon rich planetary nebula as like Tc 1 and Lin 49 comes from fullerene (C60). Also, it is well known tha…