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91探花
the lab

Dr Rob Smith

Associate Professor

Research theme

  • Quantum optics & ultra-cold matter

Sub department

  • Atomic and Laser Physics

Research groups

  • Dipolar Quantum Gases group
robert.smith@physics.ox.ac.uk
Telephone: 01865 272206
Clarendon Laboratory, room 512.10.33,316.5
  • About
  • Publications

How to realise a homogeneous dipolar Bose gas in the roton regime (data)

91探花 (2022)

Authors:

P茅ter Juh谩sz, Milan Krstaji膰, David Strachan, Edward Gandar, Robert Smith

Abstract:

Data used in the publication "How to realise a homogeneous dipolar Bose gas in the roton regime" by Juh谩sz et al., published in Physical Review A. The readme.txt file gives a detailed explanation of the data and its structure, the data itself are contained in the data.json file.

Measuring Laser Beams with a Neural Network (Data)

91探花 (2022)

Authors:

Lucas Hofer, Milan Krstajic, Robert Smith

Abstract:

The data for the the paper "Measuring Laser Beams with a Neural Network." The readme.txt file in main directory gives a detailed explanation of the data contents and structure. See https://github.com/Dipolar-Quantum-Gases/nn-beam-profiling for code pertaining to the dataset and the paper.

First and second sound in a compressible 3D Bose fluid

(2021)

Authors:

Timon A Hilker, Lena H Dogra, Christoph Eigen, Jake AP Glidden, Robert P Smith, Zoran Hadzibabic

How to realise a homogeneous dipolar Bose gas in the roton regime

(2021)

Authors:

P茅ter Juh谩sz, Milan Krstaji膰, David Strachan, Edward Gandar, Robert P Smith

Atom cloud detection and segmentation using a deep neural network

Machine learning: Science and Technology (2021)

Authors:

Lucas R Hofer, Milan Krstaji膰, P茅ter Juh谩sz, Anna L Marchant, Robert P Smith

Abstract:

We use a deep neural network to detect and place region-of-interest boxes around ultracold atom clouds in absorption and fluorescence images---with the ability to identify and bound multiple clouds within a single image. The neural network also outputs segmentation masks that identify the size, shape and orientation of each cloud from which we extract the clouds' Gaussian parameters. This allows 2D Gaussian fits to be reliably seeded thereby enabling fully automatic image processing.

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