Line nanopatterns are produced on the positive photoresist by scanning near-field optical microscope (SNOM). A laser diode with a wavelength of 450 nm and a power of 250 mW as the light source and an aluminum coated nanoprobe with a 70 nm aperture at the tip apex have been employed. A neutral density filter has been used to control the exposure power of the photoresist. It is found that the changes induced by light in the photoresist can be detected by in situ shear force microscopy (ShFM), before the development of the photoresist. Scanning electron microscope (SEM) images of the developed photoresist have been used to optimize the scanning speed and the power required for exposure, in order to minimize the final line width. It is shown that nanometric lines with a minimum width of 33 nm can be achieved with a scanning speed of 75 mu m/s and a laser power of 113 mW. It is also revealed that the overexposure of the photoresist by continuous wave laser generated heat can be prevented by means of proper photoresist selection. In addition, the effects of multiple exposures of nanopatterns on their width and depth are investigated.
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UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Credgington, Daniel
Fenwick, Oliver
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UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Fenwick, Oliver
Charas, Ana
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Inst Super Tecn, Inst Telecomunicacoes, P-1049001 Lisbon, PortugalUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Charas, Ana
Morgado, Jorge
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Inst Super Tecn, Inst Telecomunicacoes, P-1049001 Lisbon, PortugalUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Morgado, Jorge
Suhling, Klaus
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Kings Coll London, Dept Phys, London WC2R 2LS, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Suhling, Klaus
Cacialli, Franco
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UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
机构:
UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Credgington, Daniel
Fenwick, Oliver
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机构:
UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Fenwick, Oliver
Charas, Ana
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机构:
Inst Super Tecn, Inst Telecomunicacoes, P-1049001 Lisbon, PortugalUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Charas, Ana
Morgado, Jorge
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h-index: 0
机构:
Inst Super Tecn, Inst Telecomunicacoes, P-1049001 Lisbon, PortugalUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Morgado, Jorge
Suhling, Klaus
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h-index: 0
机构:
Kings Coll London, Dept Phys, London WC2R 2LS, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
Suhling, Klaus
Cacialli, Franco
论文数: 0引用数: 0
h-index: 0
机构:
UCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England
UCL, London Ctr Nanotechnol, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, CMMP Grp, London WC1E 6BT, England