Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Log inSign up
Challenges
Datasets
Workspaces
Papers
Discussions
Leaderboard
Blog
Job Board
Q3AS

© 2026 Aqora Quantum S.A.S.

TermsPrivacyLegal Notice

Bulletin of the American Physical Society

Understanding and overcoming the barriers to room-temperature quantum computation in diamond

Andrew Horsley, Sophie Stearn, Lachlan M. Oberg, Eric Huang, Neil B. Manson, Marcus W. Doherty

Published Mar 9, 2018• 0 citations
OpenAlex

Related papers

Progress towards room temperature quantum computation based on NV centers in diamond

Peter C. Maurer, Nicholas G. Chisholm, Georg Kucsko +9 more

Bulletin of the American Physical Society•May 27, 2010•1 citation

Remote Spin Coupling and Room Temperature Quantum Computation with Diamond Color Centers

Norman Y. Yao, Liang Jiang, Alexey Vyacheslavovich Gorshkov +3 more

Bulletin of the American Physical Society•May 27, 2010•0 citations

A large-scale quantum simulator on a diamond surface at room temperature

Jianming Cai, Alex Retzker, Fedor Jelezko +1 more

arXiv:1208.2874•Nature Physics•Jan 20, 2013•286 citations

Ultrafast Quantum Processing at Room-Temperature in Bulk Diamond Phonons

Benjamin Sussman, Philip J. Bustard, K.C. Lee +7 more

Bulletin of the American Physical Society•Jun 7, 2012•0 citations

Room-temperature solid-state quantum memory using pairs of nuclear spins in diamond

Nir Bar‐Gill, Stephen J. DeVience, David Le Sage +3 more

Bulletin of the American Physical Society•Feb 28, 2012•0 citations

Steady-state microwave mode cooling with a diamond NV ensemble

Donald P. Fahey, Kurt A. Jacobs, Matthew J. Turner +4 more

A fundamental result of quantum mechanics is that the fluctuations of a bosonic field are given by its temperature $T$. An electromagnetic mode with frequency $ω$ in the microwave band has a significant thermal photon occupation at room temperature according to the Bose-Einstein distribution $\bar{n} = k_BT / \hbarω$. The room temperature thermal state of a 3 GHz mode, for example, is characterized by a mean photon number $\bar{n} \sim 2000$ and variance $Δn^2 \approx \bar{n}^2$. This thermal variance sets the measurement noise floor in applications ranging from wireless communications to positioning, navigation, and timing to magnetic resonance imaging. We overcome this barrier in continuously cooling a ${\sim} 3$ GHz cavity mode by coupling it to an ensemble of optically spin-polarized nitrogen-vacancy (NV) centers in a room-temperature diamond. The NV spins are pumped into a low entropy state via a green laser and act as a heat sink to the microwave mode through their collective interaction with microwave photons. Using a simple detection circuit we report a peak noise reduction of $-2.3 \pm 0.1 \, \textrm{dB}$ and minimum cavity mode temperature of $150 \pm 5 \textrm{K}$. We present also a linearized model to identify the important features of the cooling, and demonstrate its validity through magnetically tuned, spectrally resolved measurements. The realization of efficient mode cooling at ambient temperature opens the door to applications in precision measurement and communication, with the potential to scale towards fundamental quantum limits.

arXiv:2203.03462•Mar 7, 2022•1 citation
A fundamental result of quantum mechanics is that the fluctuations of a bosonic field are given by its temperature TTT. An electromagnetic mode with frequency ωωω in the microwave band has a significant thermal photon occupation at room temperature according to the Bose-Einstein distribution nˉ=kBT/ℏω\bar{n} = k_BT / \hbarωnˉ=kB​T/ℏω. The room temperature thermal state of a 3 GHz mode, for example, is characterized by a mean photon number nˉ∼2000\bar{n} \sim 2000nˉ∼2000 and variance Δn2≈nˉ2Δn^2 \approx \bar{n}^2Δn2≈nˉ2. This thermal variance sets the measurement noise floor in applications ranging from wireless communications to positioning, navigation, and timing to magnetic resonance imaging. We overcome this barrier in continuously cooling a ∼3{\sim} 3∼3 GHz cavity mode by coupling it to an ensemble of optically spin-polarized nitrogen-vacancy (NV) centers in a room-temperature diamond. The NV spins are pumped into a low entropy state via a green laser and act as a heat sink to the microwave mode through their collective interaction with microwave photons. Using a simple detection circuit we report a peak noise reduction of −2.3±0.1 dB-2.3 \pm 0.1 \, \textrm{dB}−2.3±0.1dB and minimum cavity mode temperature of 150±5K150 \pm 5 \textrm{K}150±5K. We present also a linearized model to identify the important features of the cooling, and demonstrate its validity through magnetically tuned, spectrally resolved measurements. The realization of efficient mode cooling at ambient temperature opens the door to applications in precision measurement and communication, with the potential to scale towards fundamental quantum limits.