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This article reviews some recent developments for new cooling technologies in the fields of condensed matter physics and cold gases, both from an experimental and theoretical point of view. The main idea is to make use of distinct many-body…

Strongly Correlated Electrons · Physics 2016-01-21 Bernd Wolf , Andreas Honecker , Walter Hofstetter , Ulrich Tutsch , Michael Lang

Radiative shocks are shocks in a gas where the radiative energy and flux coming from the very hot post-shock material are non-negligible in the shock's total energy budget, and are often large enough to heat the material ahead of the shock.…

High Energy Astrophysical Phenomena · Physics 2015-06-15 N. Vaytet , M. Gonzalez , E. Audit , G. Chabrier

An ellipsoidal volume of Rydberg molecules, entrained in a supersonic molecular beam, evolves on a nanosecond timescale to form a strongly coupled ultracold plasma. We present coupled rate-equation simulations that model the underlying…

Chemical Physics · Physics 2019-08-22 Rafael Haenel , Edward Grant

Slow magnetoacoustic waves represent an important tool for probing the solar coronal plasma. We quantitatively assess the applicability of the weak thermal conduction theory to coronal seismology by slow waves. We numerically model the…

Solar and Stellar Astrophysics · Physics 2022-11-23 Dmitrii Y. Kolotkov

Local thermal instability can plausibly explain the formation of multiphase gas in many different astrophysical environments, but the theory is only well understood in the optically thin limit of the equations of radiation hydrodynamics…

High Energy Astrophysical Phenomena · Physics 2022-09-07 Daniel Proga , Tim Waters , Sergei Dyda , Zhaohuan Zhu

We develop a general method for the self consistent calculation of the hydrodynamics of an astrophysical object irradiated by a radiation field with an arbitrary strength and spectral energy distribution (SED). Using the XSTAR…

High Energy Astrophysical Phenomena · Physics 2017-03-22 Sergei Dyda , Randall Dannen , Tim Waters , Daniel Proga

How the solar corona is heated to high temperatures remains an unsolved mystery in solar physics. In the present study we analyse observations of 50 whole active-region loops taken with the Extreme-ultraviolet Imaging Spectrometer (EIS) on…

Solar and Stellar Astrophysics · Physics 2017-06-28 Haixia Xie , Maria S. Madjarska , Bo Li , Zhenghua Huang , Lidong Xia , Thomas Wiegelmann , Hui Fu , Chaozhou Mou

We present a new scenario for the formation of cool cores in rich galaxy clusters based on results from recent high spatial dynamic range, adaptive mesh Eulerian hydrodynamic simulations of large-scale structure formation. We find that…

Astrophysics · Physics 2008-11-26 Patrick M. Motl , Jack O. Burns , Chris Loken , Michael L. Norman , Greg Bryan

We present a laser cooling scheme for trapped ions and atoms using a combination of laser couplings and a magnetic gradient field. In a Schrieffer-Wolff transformed picture, this setup cancels the carrier and blue sideband terms completely…

Quantum Physics · Physics 2011-03-18 Andreas Albrecht , Alex Retzker , Christof Wunderlich , Martin B. Plenio

Accelerated cooling is a key technology in producing thermomechanically controlled processed (TMCP) steel plates. In a TMCP process hot plates are subjected to a strong cooling what results in a complex microstructure leading to increased…

Numerical Analysis · Mathematics 2019-12-30 Dimitri Rothermel , Thomas Schuster , Roland Schorr , Martin Peglow

In collisional ionization equilibrium (CIE), the X-ray spectrum from a plasma depends on the distribution of emission measure over temperature (DEM). Due to the well-known ill conditioning problem, no precisely resolved DEM can be inverted…

High Energy Astrophysical Phenomena · Physics 2014-01-28 K. G. Gayley

We develop a new algorithm to estimate the temperature of a nonneutral plasma in a Penning-Malmberg trap. The algorithm analyzes data obtained by slowly lowering a voltage that confines one end of the plasma and collecting escaping charges,…

Plasma Physics · Physics 2024-09-19 Adrianne Zhong , Joel Fajans , Jonathan S. Wurtele

The ASACUSA collaboration produces a beam of antihydrogen atoms by mixing pure positron and antiproton plasmas in a strong magnetic field with a double cusp geometry. The positrons cool via cyclotron radiation inside the cryogenic trap. Low…

Cooling microwave resonators to near the quantum ground state, crucial for their operation in the quantum regime, is typically achieved by direct device refrigeration to a few tens of millikelvin. However, in quantum experiments that…

Quantum Physics · Physics 2020-01-29 Mingrui Xu , Xu Han , Chang-Ling Zou , Wei Fu , Yuntao Xu , Changchun Zhong , Liang Jiang , Hong X. Tang

The heating of particles by plasma radiation plays a critical role in space science involving dusty plasma as well as in industrial processes such as plasma vapor deposition, microchip production, etching and plasma fusion. Numerical…

Plasma Physics · Physics 2025-09-09 A. Povitsky , M. N. Shneider

Molecular dynamics simulations are used to model ion and neutral temperature evolution in partially-ionized atmospheric pressure plasma at different ionization fractions. Results show that ion-ion interactions are strongly coupled at…

Plasma Physics · Physics 2023-01-04 M. D. Acciarri , C. Moore , S. D. Baalrud

Radiative processes play a pivotal role in shaping the thermal and chemical states of gas across diverse astrophysical environments, from the interstellar medium (ISM) to the intergalactic medium. We present a hybrid cooling model for…

New results from MAST are presented that focus on validating models in order to extrapolate to future devices. Measurements during start-up experiments have shown how the bulk ion temperature rise scales with the square of the reconnecting…

Plasma Physics · Physics 2017-08-02 A Kirk , J Adamek , RJ Akers , S Allan , L Appel , F Arese Lucini , M Barnes , T Barrett , N Ben Ayed , W Boeglin , J Bradley , P K Browning , J Brunner , P Cahyna , M Carr , F Casson , M Cecconello , C Challis , IT Chapman , S Chapman , S Conroy , N Conway , WA Cooper , M Cox , N Crocker , B Crowley , S Cardnell , J Chorley , G Cunningham , A Danilov , D Darrow , R Dendy , D Dickinson , W Dorland , B Dudson , L Easy , S Elmore , M Evans , T Farley , N Fedorczak , A Field , I Fitzgerald , M Fox , S Freethy , L Garzotti , YC Ghim , K Gi , M Gorelenkova , W Gracias , C Gurl , W Guttenfelder , C Ham , D Harting , E Havlickova , N Hawkes , T Hender , S Henderson , J Hillesheim , B Hnat , J Horacek , J Howard , D Howell , D Dunai , G Fishpool , K Gibson , J Harrison , E Highcock , B Huang , M Inomoto , R Imazawa , O Jones , K Kadowaki , S Kaye , D Keeling , M Kocan , L Kogan , M Komm , W Lai , J Leddy , H Leggate , K Imada , I Klimek , J Hollocombe , B Lipschultz , S Lisgo , YQ Liu , B Lloyd , B Lomanowski , V Lukin , G Maddison , J Madsen , J Mailloux , R Martin , G McArdle , I Lupelli , K McClements , B McMillan , A Meakins , H Meyer , C Michael , F Militello , J Milnes , G Motojima , D Muir , G Naylor , A Nielsen , M O'Brien , M O'Mullane , J Olsen , J Omotani , Y Ono , S Pamela , AW Morris , T O'Gorman , L Pangione , F Parra , A Patel , W Peebles , R Perez , S Pinches , L Piron , M Price , M Reinke , P Ricci , F Riva , C Roach , M Romanelli , D Ryan , S Saarelma , A Saveliev , R Scannell , A Schekochihin , S Sharapov , R Sharples , V Shevchenko , K Shinohara , S Silburn , J Simpson , A Stanier , J Storrs , H Summers , Y Takase , P Tamain , H Tanabe , H Tanaka , K Tani , D Taylor , D Thomas , N Thomas-Davies , A Thornton , M Turnyanskiy , M Valovic , R Vann , F Van Wyk , N Walkden , T Watanabe , H Wilson , M Wischmeier , T Yamada , J Young , S Zoletnik , the MAST Team , the EUROfusion MST1 Team

Numerical modeling of the edge and scrape-off layer (SOL) must account for atomic processes such as hydrogenic ionization and recombination, charge-exchange, and line radiation. Their reaction rates depend non-linearly on density and…

Plasma Physics · Physics 2026-04-01 Konrad Eder , Wladimir Zholobenko , Andreas Stegmeir , Kaiyu Zhang , Frank Jenko

Radio Frequency (RF) driven helicon plasma sources are commonly used for their ability to produce high-density argon plasmas (n > 10^19/m^3) at relatively moderate powers (typical RF power < 2 kW). Typical electron temperatures are < 10 eV…