One-click electromagnetism at the nanoscale

Platinum nanoparticle UV-vis spectrum calculator

Questions & answers

Do platinum nanoparticles have a plasmon peak?

Not in the visible. Platinum's strong interband absorption damps its plasmon so much that the UV-vis spectrum of particles under about 60 nm is featureless, rising towards the UV. Only large particles (80 nm and up) show a broad maximum, from scattering: about 414 nm at 80 nm and 448 nm at 100 nm (table above).

Why are platinum nanoparticle colloids dark brown or black?

They absorb across the whole visible range without a resonance to pick out one colour, so a colloid darkens from brown to black as the concentration grows.

How do I find the concentration of platinum nanoparticles from UV-vis?

Use the extinction at a fixed wavelength, for example 400 nm, and the molar extinction coefficient for your size from the table (about 4.2 × 108 M−1 cm−1 at 400 nm for 20 nm spheres): c = A / (ε ℓ). The calculator gives ε at any wavelength from Cext.

Are platinum nanoparticles good for photothermal heating?

They absorb broadband light efficiently, so they heat under white light or lasers of any colour, but without the resonant boost of gold. The nanoparticle heating calculator gives the temperature rise for any material and size.

Can I compute platinum nanospheres, core–shell nanoparticles, arrays, near fields, heating or substrates?

Yes: platinum nanospheres and core–shell nanoparticles (add a shell) are available in every calculator, from spectra to optical properties: near-field enhancement maps, dimers and hot spots, nanoparticle arrays and lattice resonances, particles on a substrate, emitters and the Purcell factor, nanorods and laser heating.

Extinction (UV-vis), absorption and scattering spectra of platinum nanospheres of any size, in any medium, in one click, from exact Mie theory.

Platinum nanoparticle size vs UV-vis spectrum

Platinum spheres in water, from exact Mie theory with this site's solver. Small platinum particles have no peak in the visible; their extinction rises steadily into the UV.

DiameterVisible maximumMolar extinction coefficientScattering share
5 nmnone: featureless5.80 × 106 M−1 cm−1< 1 %
10 nmnone: featureless4.74 × 107 M−1 cm−1< 1 %
20 nmnone: featureless4.15 × 108 M−1 cm−12 %
30 nmnone: featureless1.64 × 109 M−1 cm−18 %
40 nmnone: featureless4.82 × 109 M−1 cm−116 %
50 nmnone: featureless1.19 × 1010 M−1 cm−127 %
60 nmnone: featureless2.46 × 1010 M−1 cm−138 %
80 nm414 nm6.22 × 1010 M−1 cm−160 %
100 nm448 nm9.83 × 1010 M−1 cm−178 %
150 nm568 nm1.75 × 1011 M−1 cm−193 %
200 nm732 nm2.69 × 1011 M−1 cm−196 %

Platinum optical constants: Werner et al. (2009); water: Hale & Querry (1973). Molar extinction coefficient at 400 nm for the featureless spectra, at the maximum otherwise; ε = NA Cext / (1000 ln 10). The broad maximum of large particles is a scattering resonance.

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