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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Peter Hatfield

Visitor

Research theme

  • Astronomy and astrophysics
  • Lasers and high energy density science

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
peter.hatfield@physics.ox.ac.uk
  • About
  • Publications

The data-driven future of high energy density physics

ArXiv 2111.1131 (2021)

Authors:

Peter W Hatfield, Jim A Gaffney, Gemma J Anderson, Suzanne Ali, Luca Antonelli, Suzan Ba艧e臒mez du Pree, Jonathan Citrin, Marta Fajardo, Patrick Knapp, Brendan Kettle, Bogdan Kustowski, Michael J MacDonald, Derek Mariscal, Madison E Martin, Taisuke Nagayama, Charlotte AJ Palmer, J Luc Peterson, Steven Rose, JJ Ruby, Carl Shneider, Matt JV Streeter, Will Trickey, Ben Williams

A laser鈥損lasma platform for photon鈥損hoton physics: the two photon Breit鈥揥heeler process

New Journal of Physics IOP Publishing 23 (2021) 115006

Authors:

B Kettle, D Hollatz, E Gerstmayr, Gm Samarin, A Alejo, S Astbury, C Baird, S Bohlen, M Campbell, C Colgan, D Dannheim, C Gregory, H Harsh, P Hatfield, J Hinojosa, Y Katzir, J Morton, Cd Murphy, A Nurnberg, J Osterhoff, G P茅rez-Callejo, K Poder, Pp Rajeev, C Roedel, F Roeder, Fc Salgado, G Sarri, A Seidel, S Spannagel, C Spindloe, S Steinke, Mjv Streeter, Agr Thomas, C Underwood, R Watt, M Zepf, Sj Rose, Spd Mangles

Abstract:

We describe a laser鈥損lasma platform for photon鈥損hoton collision experiments to measure fundamental quantum electrodynamic processes. As an example we describe using this platform to attempt to observe the linear Breit鈥揥heeler process. The platform has been developed using the Gemini laser facility at the Rutherford Appleton Laboratory. A laser Wakefield accelerator and a bremsstrahlung convertor are used to generate a collimated beam of photons with energies of hundreds of MeV, that collide with keV x-ray photons generated by a laser heated plasma target. To detect the pairs generated by the photon鈥損hoton collisions, a magnetic transport system has been developed which directs the pairs onto scintillation-based and hybrid silicon pixel single particle detectors (SPDs). We present commissioning results from an experimental campaign using this laser鈥損lasma platform for photon鈥損hoton physics, demonstrating successful generation of both photon sources, characterisation of the magnetic transport system and calibration of the SPDs, and discuss the feasibility of this platform for the observation of the Breit鈥揥heeler process. The design of the platform will also serve as the basis for the investigation of strong-field quantum electrodynamic processes such as the nonlinear Breit鈥揥heeler and the Trident process, or eventually, photon鈥損hoton scattering.

The LSST-DESC 3x2pt tomography optimization challenge

The Open Journal of Astrophysics Maynooth Academic Publishing 4:1 (2021)

Authors:

Joe Zuntz, Fran莽ois Lanusse, Alex I Malz, Angus H Wright, An啪e Slosar, Bela Abolfathi, David Alonso, Abby Bault, Cl茅cio R Bom, Massimo Brescia, Adam Broussard, Jean-Eric Campagne, Stefano Cavuoti, Eduardo S Cypriano, Bernardo MO Fraga, Eric Gawiser, Elizabeth J Gonzalez, Dylan Green, Peter Hatfield, Kartheik Iyer, David Kirkby, Andrina Nicola, Erfan Nourbakhsh, Andy Park, Gabriel Teixeira, Katrin Heitmann, Eve Kovacs, Yao-Yuan Mao

Abstract:

This paper presents the results of the Rubin Observatory Dark Energy Science Collaboration (DESC) 3x2pt tomography challenge, which served as a first step toward optimizing the tomographic binning strategy for the main DESC analysis. The task of choosing an optimal tomographic binning scheme for a photometric survey is made particularly delicate in the context of a metacalibrated lensing catalogue, as only the photometry from the bands included in the metacalibration process (usually riz and potentially g) can be used in sample definition. The goal of the challenge was to collect and compare bin assignment strategies under various metrics of a standard 3x2pt cosmology analysis in a highly idealized setting to establish a baseline for realistically complex follow-up studies; in this preliminary study, we used two sets of cosmological simulations of galaxy redshifts and photometry under a simple noise model neglecting photometric outliers and variation in observing conditions, and contributed algorithms were provided with a representative and complete training set. We review and evaluate the entries to the challenge, finding that even from this limited photometry information, multiple algorithms can separate tomographic bins reasonably well, reaching figures-of-merit scores close to the attainable maximum. We further find that adding the g band to riz photometry improves metric performance by ~15% and that the optimal bin assignment strategy depends strongly on the science case: which figure-of-merit is to be optimized, and which observables (clustering, lensing, or both) are included.

MIGHTEE-H鈥塈: the baryonic Tully鈥揊isher relation over the last billion years

Monthly Notices of the Royal Astronomical Society 91探花 University Press 508:1 (2021) 1195-1205

Authors:

Anastasia A Ponomareva, Wanga Mulaudzi, Natasha Maddox, Bradley S Frank, Matt J Jarvis, Enrico M Di Teodoro, Marcin Glowacki, Renee C Kraan-Korteweg, Tom A Oosterloo, Elizabeth AK Adams, Hengxing Pan, Isabella Prandoni, Sambatriniaina HA Rajohnson, Francesco Sinigaglia, Nathan J Adams, Ian Heywood, Rebecca AA Bowler, Peter W Hatfield, Jordan D Collier, Srikrishna Sekhar

Abstract:

Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H i-based baryonic Tully-Fisher relation (bTFr), covering a period of ∼1 billion years (0 ≤ z ≤ 0.081). We consider the bTFr based on two different rotational velocity measures: The width of the global H i profile and Vout, measured as the outermost rotational velocity from the resolved H i rotation curves. Both relations exhibit very low intrinsic scatter orthogonal to the best-fitting relation (σ⊥ = 0.07 ± 0.01), comparable to the SPARC sample at z 0. The slopes of the relations are similar and consistent with the z 0 studies (3.66+0.35-0.29 for W50 and 3.47+0.37-0.30 for Vout). We find no evidence that the bTFr has evolved over the last billion years, and all galaxies in our sample are consistent with the same relation independent of redshift and the rotational velocity measure. Our results set-up a reference for all future studies of the H i-based bTFr as a function of redshift that will be conducted with the ongoing deep SKA pathfinders surveys.

Astronomy Domine: advancing science with a burning plasma

Contemporary Physics Taylor & Francis (2021)

Authors:

steven Rose, PETER HATFIELD

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