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Jonathan Breeze, Neil Alford, et al [Imperial + UCL] collaboration

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Presentation on theme: "Jonathan Breeze, Neil Alford, et al [Imperial + UCL] collaboration"— Presentation transcript:

1 Jonathan Breeze, Neil Alford, et al [Imperial + UCL] collaboration
Quantum Microwave Technology –MASERs and beyond Mark Oxborrow NV diamond Maser oscillation, continuous, solid-state, room temperature Jonathan Breeze, Neil Alford, et al [Imperial + UCL] collaboration

2 “Microwaves” oven magnetron radar

3 Microwaves one the Electromagnetic Spectrum
Maxwell Hertz Visible light Microwaves λ = 10 cm λ = cm Factor of 100,000 in wavelength (or frequency)

4 Waves behaving badly …. like particles (“quanta”)

5 Getting Inside Your Head (with MRI, EPR, Endor … )
Philips MRI Microwaves refresh the parts wot other photons cannot reach.

6 ? Doing “Quantum Optics” ( Quantum Technologies)
Counting/detecting single photons energy of a photon Optical wavelengths: Microwaves: ? 100,000 times less energy per photon photomultipliers Difficult! avalanche photodiodes

7 The Bad News: Thermal Photons
At room temperature, number of microwave photons in an electromagnetic 10 GHz 300 microwave photon

8 The Good News: Spontaneous Emission
Rate of spontaneous emission Einstein’s A coefficient (causing shot noise) extremely low (too small to care about)

9 Cooling to Photonic Ground State (at room temperature)
NV diamond Microwave wave transition with equivalent Boltzmamn temperature of ~100 mK 3 GHz

10 Look to the Heavens! Sky Temperature Frequency

11 Avalanche Photo-detector for Microwave Photons
pentacene:p-terphenyl Main reference: “Room-temperature solid-state maser”, M. Oxborrow, J. D. Breeze and N. M. Alford, Nature 488, (2012).

12 Quantum Microwave Technology in a Nutshell:
Every photon’s precious. Every photon counts. If you can count microwaves, in the bank comes large amounts. picking a pocket or two …


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