M. P. Böhme, L. B. Fletcher, A. D. Baczewski, H. M. Bellenbaum, Z. A. Moldabekov, J. Vorberger, D. A. Chapman, M. J. MacDonald, S. Schwalbe, T. R. Preston, D. Kraus, T. Gawne, F. R. Graziani, S. Hamel, T. Döppner, T. Dornheim
{"title":"Evidence of Free-Bound Transitions in Warm Dense Matter and Their Impact on Equation-of-State Measurements","authors":"M. P. Böhme, L. B. Fletcher, A. D. Baczewski, H. M. Bellenbaum, Z. A. Moldabekov, J. Vorberger, D. A. Chapman, M. J. MacDonald, S. Schwalbe, T. R. Preston, D. Kraus, T. Gawne, F. R. Graziani, S. Hamel, T. Döppner, T. Dornheim","doi":"10.1002/ctpp.70149","DOIUrl":"https://doi.org/10.1002/ctpp.70149","url":null,"abstract":"<p>Warm dense matter (WDM) is now routinely created and probed in laboratories around the world, providing unprecedented insights into conditions achieved in stellar atmospheres, planetary interiors, and inertial confinement fusion experiments. However, the interpretation of these experiments is often filtered through models with systematic errors that are difficult to quantify. Due to the simultaneous presence of quantum degeneracy and thermal excitation, transitions in which free electrons are de-excited into thermally unoccupied bound states transferring momentum and energy to a scattered x-ray photon become viable. Here we show that such <i>free-bound</i> transitions are a particular feature of WDM and vanish in the limits of cold and hot temperatures. The inclusion of these transitions into the analysis of recent X-ray Thomson Scattering experiments on WDM at the National Ignition Facility and the Linac Coherent Light Source is required to obtain a physically consistent temperature from the Chihara decomposition. This interpretation is corroborated by agreement with a recently developed model-free thermometry technique and presents an important step for precisely characterizing and understanding the complex WDM state of matter.</p>","PeriodicalId":10700,"journal":{"name":"Contributions to Plasma Physics","volume":"66 7-8","pages":""},"PeriodicalIF":1.1,"publicationDate":"2026-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1002/ctpp.70149","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149072604","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Jan-Philip Joost, Christopher Makait, Alexander Osterkorn, Erik Schroedter
{"title":"Quenching the Hubbard Model: Comparison of Nonequilibrium Green's Function Methods","authors":"Jan-Philip Joost, Christopher Makait, Alexander Osterkorn, Erik Schroedter","doi":"10.1002/ctpp.70075","DOIUrl":"https://doi.org/10.1002/ctpp.70075","url":null,"abstract":"<p>We benchmark nonequilibrium Green's function (NEGF) approaches for interaction quenches in the half-filled Fermi–Hubbard model in one and two dimensions. We compare fully self-consistent two-time Kadanoff–Baym equations (KBE), the generalized Kadanoff–Baym ansatz (GKBA), and the recently developed NEGF-based quantum fluctuations approach (NEGF-QF) with second-order Born (2B) and <i>GW</i> self-energies. As references, we use DMRG in 1D and time-dependent perturbation theory at weak coupling. While all methods reproduce the early-time build-up of correlations (prethermalization), different deficiencies emerge during the slower relaxation in the long-time limit: KBE shows overdamped oscillations, GKBA exhibits a negative overshoot of the Fermi-surface jump, and NEGF-QF develops a prethermalization plateau with delayed relaxation. In 1D, we find that GKBA + 2B agrees best with DMRG across the explored parameter range, while QF + <i>GW</i> deviates the most, consistent with its reduced self-consistency. In 2D, all approaches correctly capture the momentum-dependence of the relaxation dynamics.</p>","PeriodicalId":10700,"journal":{"name":"Contributions to Plasma Physics","volume":"66 7-8","pages":""},"PeriodicalIF":1.1,"publicationDate":"2026-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1002/ctpp.70075","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149072611","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Heather D. Whitley, Michael S. Murillo, John I. Castor, Liam G. Stanton, Lorin X. Benedict, Philip A. Sterne, James N. Glosli, Frank R. Graziani
{"title":"Improved Kelbg Potentials for \u0000 \u0000 \u0000 Z\u0000 >\u0000 1\u0000 \u0000 $$ Z>1 $$\u0000 and Application to Carbon Plasmas","authors":"Heather D. Whitley, Michael S. Murillo, John I. Castor, Liam G. Stanton, Lorin X. Benedict, Philip A. Sterne, James N. Glosli, Frank R. Graziani","doi":"10.1002/ctpp.70130","DOIUrl":"https://doi.org/10.1002/ctpp.70130","url":null,"abstract":"<div>\u0000 \u0000 <p>In this work, we present a general form for the electron-ion diffractive potential derived from the quantum pair density matrix and fit to the improved Kelbg potential for atomic numbers up to <span></span><math>\u0000 <semantics>\u0000 <mrow>\u0000 <mi>Z</mi>\u0000 <mo>=</mo>\u0000 <mn>54</mn>\u0000 </mrow>\u0000 <annotation>$$ Z=54 $$</annotation>\u0000 </semantics></math>. We apply classical molecular dynamics using the improved Kelbg potential for carbon with various forms of the Pauli potential to compute internal energies and pressures for hot, dense plasma conditions. Our results are compared to an equation of state model based on path integral Monte Carlo and density functional theory simulations to examine the extent to which the improved Kelbg potential reproduces the internal energy and pressure of carbon plasmas. The regions of validity for carbon agree generally with those derived previously for hydrogen once pressure ionization effects are incorporated. Based on our carbon results and previously published hydrogen studies, we discuss the general applicability and limitations of these potentials for equation of state studies in warm dense matter and high energy density plasmas.</p>\u0000 </div>","PeriodicalId":10700,"journal":{"name":"Contributions to Plasma Physics","volume":"66 7-8","pages":""},"PeriodicalIF":1.1,"publicationDate":"2026-09-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"149072723","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}