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Stable ensemble brightness from nitrogen vacancy centers in nanodiamonds through optimized surface composition


Affiliations
1 CSIR-National Physical Laboratory, Dr K S Krishnan Marg, New Delhi 110 012, India
2 Academy of Scientific and Innovative Research (AcSIR), Ghaziabad, Uttar Pradesh 201 002, India
3 Inter University Accelerator Centre, Aruna Asaf Ali Marg, New Delhi 110 067, India

Stable ensemble emission from nitrogen vacancy (NV) centers in nanodiamonds (NDs) is highly desirable for diverse areas ranging from bio-imaging to quantum optics. The uniqueness of NV centers lies in their opto-spin properties like energy level structure, emission range (620-850 nm) and optical spin polarization. The host matrix (NDs), however, put some limitation on the photo-physical properties of these color centers. One of the major issues is surface proximity (where high concentration of defects are present) of NV centers. The NV centers being highly sensitive to the neighboring environment are unstable in such circumstances. The surface of NDs mainly exhibit non-diamond carbon which is well-known quencher of emission due to NV centers. The surface composition for desirable photo-physical properties of NV centers is still unknown. Here, we have systemically studied the effect of oxidation time at low oxidation temperature (450 oC) on the selective removal of sp2 carbon, aqueous dispersion of NDs and emission collection due to NV centers at ensemble level. Among different air oxidations, heat treatment at 450 oC at residual time of 8 hours has been found to be suitable air oxidation conditions for the enhancement of brightness and ensemble photo-stability of NV centers.
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  • Stable ensemble brightness from nitrogen vacancy centers in nanodiamonds through optimized surface composition

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Authors

Sandeep
CSIR-National Physical Laboratory, Dr K S Krishnan Marg, New Delhi 110 012, India
Ravi Kumar
Academy of Scientific and Innovative Research (AcSIR), Ghaziabad, Uttar Pradesh 201 002, India
Ravi Kumar
CSIR-National Physical Laboratory, Dr K S Krishnan Marg, New Delhi 110 012, India
Kiran Mahadeo Subhedar
Academy of Scientific and Innovative Research (AcSIR), Ghaziabad, Uttar Pradesh 201 002, India
Kiran Mahadeo Subhedar
CSIR-National Physical Laboratory, Dr K S Krishnan Marg, New Delhi 110 012, India
Raj Kumar
Inter University Accelerator Centre, Aruna Asaf Ali Marg, New Delhi 110 067, India
Sanjay Rangnath Dhakate
Academy of Scientific and Innovative Research (AcSIR), Ghaziabad, Uttar Pradesh 201 002, India
Sanjay Rangnath Dhakate
CSIR-National Physical Laboratory, Dr K S Krishnan Marg, New Delhi 110 012, India

Abstract


Stable ensemble emission from nitrogen vacancy (NV) centers in nanodiamonds (NDs) is highly desirable for diverse areas ranging from bio-imaging to quantum optics. The uniqueness of NV centers lies in their opto-spin properties like energy level structure, emission range (620-850 nm) and optical spin polarization. The host matrix (NDs), however, put some limitation on the photo-physical properties of these color centers. One of the major issues is surface proximity (where high concentration of defects are present) of NV centers. The NV centers being highly sensitive to the neighboring environment are unstable in such circumstances. The surface of NDs mainly exhibit non-diamond carbon which is well-known quencher of emission due to NV centers. The surface composition for desirable photo-physical properties of NV centers is still unknown. Here, we have systemically studied the effect of oxidation time at low oxidation temperature (450 oC) on the selective removal of sp2 carbon, aqueous dispersion of NDs and emission collection due to NV centers at ensemble level. Among different air oxidations, heat treatment at 450 oC at residual time of 8 hours has been found to be suitable air oxidation conditions for the enhancement of brightness and ensemble photo-stability of NV centers.