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We report a first-principles density functional theory study on the role of grain boundary and dislocation loop in H blistering in W. At low temperature, the {\Sugma}3(111) tilt grain boundary, when combined with a vacancy of vanishing…

Materials Science · Physics 2015-05-27 W. Xiao , W. T. Geng

We present a detailed first principles density functional theory study of intrinsic and extrinsic point defects in monolayer (ML) WSe2. Among the intrinsic point defects, Se vacancies (Sevac) have the lowest formation energy (disregarding…

Materials Science · Physics 2019-01-17 Yu Jie Zheng , Su Ying Quek

With the first principles calculations of H and He induced energetics change we demonstrate that in W the accumulation of H (up to 9) and He (up to 4) in a single vacancy (V) surprisingly reduce the formation energy of first and second…

Materials Science · Physics 2013-05-03 Yu-Wei You , Xiang-Shan Kong , Q. F. Fang , Jun-Ling Chen , G. -N. Luo , C. S. Liu , B. C. Pan , Y. Daid

Methods: The microscopic equations of H2-formation and protonation are integrated numerically over time in such a manner that the overall structures evolve self-consistently under benign conditions. Results: The equilibrium H2 formation…

Astrophysics of Galaxies · Physics 2009-11-13 H. S. Liszt

The mean energy $W$ required to produce an ion pair in molecular hydrogen has been obtained for protons in the energy range between 1 MeV and 4.5 MeV. The W values were derived from the existing experimental data on elastic {\it $\pi^-$p}…

Instrumentation and Detectors · Physics 2014-05-23 G. A. Korolev , G. D. Alkhazov , A. V. Dobrovolsky , A. V. Khanzadeev , A. A. Vorobyov

Charge density wave (CDW) is a collective quantum phenomenon with a charge modulation in solids1-2. Condensation of electron and hole pairs with finite momentum will lead to such an ordered state3-7. However, lattice symmetry breaking…

Helium (He) retention in tungsten (W) is a concern in fusion reactors since it could be detrimental to plasma facing components performance and influence the fusion fuel balance. He being not soluble in W, it tends to agglomerate on…

Chemical Physics · Physics 2022-12-07 A. Dunand , M. Minissale , T. Angot , R. Bisson

The behaviors of hydrogen (H) in MAX phase material Ti3SiC2 have been investigated using first-principles method. We show that a single H atom prefers to stay 1.01 {\AA} down of the Si vacancy with solution energy of about -4.07 eV,…

Materials Science · Physics 2013-08-06 Yi-Guo Xu , Xue-Dong Ou , Xi-Ming Rong

Ni-W based medium heavy alloys offer a promising pathway to bridge the density-strength gap between tungsten heavy alloys and ultrahigh-strength steels. In this study, the effects of W concentration on short-range order (SRO), deformation…

WW scattering is an important process to study electroweak symmetry breaking in the Standard Model at the LHC, in which the Higgs mechanism or other new physics processes must intervene to preserve the unitarity of the process below 1 TeV.…

High Energy Physics - Experiment · Physics 2011-02-09 Bo Zhu , Pietro Govoni , Yajun Mao , Chiara Mariotti , Weimin Wu

The stability and formation mechanism of the defects relevant to silicon and carbon vacancies at the 4H-SiC(000$\bar{1}$)/SiO$_2$ interface after wet oxidation are investigated by first-principles calculation based on the density functional…

Materials Science · Physics 2024-01-09 Mukai Tsunasaki , Tomoya Ono , Mitsuharu Uemoto

Properties of point defects resulting from the incorporation of inert-gas atoms in bcc tungsten are investigated systematically using first-principles density functional theory (DFT) calculations. The most stable configuration for the…

Materials Science · Physics 2015-10-29 Duc Nguyen-Manh , S. L. Dudarev

Condensation of H 2 in the interstellar medium (ISM) has long been seen as a possibility, either by deposition on dust grains or thanks to a phase transition combined with self-gravity. H 2 condensation might explain the observed low…

Astrophysics of Galaxies · Physics 2018-06-06 Andreas Füglistaler , Daniel Pfenniger

The Bose-Einstein condensation of excitons continues to garner immense attention as a prototypical example for observing emergent properties from many-body quantum effects. In particular, Titanium Diselenide (TiSe$_2$) is a promising…

Materials Science · Physics 2019-12-06 Chao Lian , Zulfikhar A. Ali , Bryan M. Wong

We use far-UV absorption spectra obtained with FUSE towards three late B stars to study the formation and excitation of H2 in the diffuse ISM. The data interpretation relies on a model of the chemical and thermal balance in…

W and W-based high-entropy alloys (HEAs) are promising candidates for plasma-facing materials in fusion reactors. While irradiation studies on W have revealed a tendency for helium (He) bubble formation and radiation-induced defects,…

Materials Science · Physics 2025-11-04 Amin Esfandiarpour , Damian Kalita , Zbigniew Koziol , Mikko Alava

We present numerical computations and analysis of atomic to molecular (HI-to-H$_2$) transitions in cool ($\sim$100 K) low-metallicity dust-free (primordial) gas, in which molecule formation occurs via cosmic-ray driven negative ion…

Astrophysics of Galaxies · Physics 2021-10-27 Amiel Sternberg , Alon Gurman , Shmuel Bialy

The ability of primordial gas to cool in proto-galactic haloes exposed to Lyman-Werner (LW) radiation is critically dependent on the self-shielding of H_2. We perform radiative transfer calculations of LW line photons, post-processing…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Jemma Wolcott-Green , Zoltán Haiman , Greg L. Bryan

Point defect species and concentrations in metastable Fe-C alloys are determined using density functional theory and a constrained free-energy functional. Carbon interstitials dominate unless iron vacancies are in significant excess,…

Materials Science · Physics 2007-05-23 Clemens J. Foerst , Jan Slycke , Krystyn J. Van Vliet , Sidney Yip

C$^+$ is a critical constituent of many regions of the interstellar medium, as it can be a major reservoir of carbon and, under a wide range of conditions, the dominant gas coolant. Emission from its 158$\mu$m fine structure line is used to…

Astrophysics of Galaxies · Physics 2019-08-19 Laurent Wiesenfeld , Paul F. Goldsmith
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