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Related papers: H$_2$ ortho-para spin conversion on inhomogeneous …

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Water, H$_2$O, is one of the fundamental molecules in chemistry, biology and astrophysics. It exists as two distinct nuclear-spin isomers, para- and ortho-water, which do not interconvert in isolated molecules. The experimental challenges…

Chemical Physics · Physics 2018-07-04 Ardita Kilaj , Hong Gao , Daniel Rösch , Uxia Rivero , Jochen Küpper , Stefan Willitsch

We discuss the notions of spin-orbital polarization and ordering in paramagnetic materials, and address their consequences in transition metal oxides. Extending the combined density functional and dynamical mean field theory scheme to the…

Strongly Correlated Electrons · Physics 2014-12-16 Cyril Martins , Markus Aichhorn , Loig Vaugier , Silke Biermann

Iron sesquioxide (Fe2O3) displays pressure and temperature induced spin and structural transitions. Our calculations show that, density functional theory (DFT), in the generalized gradient approximation (GGA) scheme, is capable of capturing…

Materials Science · Physics 2009-05-22 Dipta Bhanu Ghosh , Stefano de Gironcoli

The formation of stars and planetary systems is a complex phenomenon, which relies on the interplay of multiple physical processes. Nonetheless, it represents a crucial stage for our understanding of the Universe, and in particular of the…

Astrophysics of Galaxies · Physics 2022-01-05 Alessandro Lupi , Stefano Bovino , Tommaso Grassi

$^{75}$As NMR measurements were performed on a polycrystalline sample of spin-1/2 alternating-spin-chain Heisenberg antiferromagnet AgVOAsO$_4$. Temperature-dependent NMR shift $K(T)$, which is a direct measure of the intrinsic spin…

Materials Science · Physics 2017-12-27 N. Ahmed , P. Khuntia , H. Rosner , M. Baenitz , A. A. Tsirlin , R. Nath

We consider $h$-stable local optima of Ising spin glass models, defined as spin configurations such that for nearly all of the spins, flipping their values results in increasing energy by at least a given amount $h$. Spins satisfying this…

Probability · Mathematics 2025-09-10 Yatin Dandi , David Gamarnik , Lenka Zdeborová

We extend our recent theoretical work on the bending relaxation of H$_2$O in collisions with H$_2$ by including the three water modes of vibration coupled with rotation, as well as the rotation of H$_2$. Our full quantum close-coupling…

Chemical Physics · Physics 2023-11-16 Ricardo Manuel Garcia-Vazquez , Alexandre Faure , Thierry Stoecklin

Nonthermal desorption of molecules from icy grain surfaces is required to explain molecular line observations in the cold gas of star-forming regions. Chemical desorption is one of the nonthermal desorption processes and is driven by the…

Astrophysics of Galaxies · Physics 2022-03-02 Kenji Furuya , Yasuhiro Oba , Takashi Shimonishi

We have performed an experimental and theoretical investigation on the spin reorientation transitions Ho$_{1-y}$Gd$_y$Al$_2$ compounds. Crystallographic, magnetic and calorimetric measurements have been performed for five selected samples…

Materials Science · Physics 2020-11-06 V. S. R. De Sousa , L. E. L. Silva , A. M. Gomes , P. J. von Ranke

One of the remaining issues concerning the spin-triplet superconductivity of Sr2RuO4 is the strong limit of the in-plane upper critical field Hc2 at low temperatures. In this study, we clarified the dependence of Hc2 on the angle theta…

Superconductivity · Physics 2009-11-16 S. Kittaka , T. Nakamura , Y. Aono , S. Yonezawa , K. Ishida , Y. Maeno

We discuss the dynamics of dust grains subjected to uncompensated torques arising from H_2 formation. In particular, we discuss grain dynamics when a grain spins down and goes through a ``crossover''. As first pointed out by Spitzer &…

Astrophysics · Physics 2009-10-28 A. Lazarian , B. T. Draine

We introduce and test a new and highly efficient method for treating the thermal and radiative effects influencing the energy equation in SPH simulations of star formation. The method uses the density, temperature and gravitational…

Astrophysics · Physics 2009-11-13 D. Stamatellos , A. P. Whitworth , T. Bisbas , S. Goodwin

Binding energies (BEs) of adsorbates on interstellar dust grains critically control adsorption, desorption, diffusion, and surface reactivity, and therefore strongly influence astrochemical models of star- and planet-forming regions. While…

Chemical Physics · Physics 2026-02-12 Anant Vaishnav , Niels M. Mikkelsen , Mie Andersen

The influence of a dust grain mixture consisting of spherical dust grains with different radii and/or chemical composition on the resulting temperature structure and spectral energy distribution of a circumstellar shell is investigated. The…

Astrophysics · Physics 2009-11-07 S. Wolf

Planet atmosphere and hydrosphere compositions are fundamentally set by accretion of volatiles, and therefore by the division of volatiles between gas and solids in planet-forming disks. For hyper-volatiles such as CO, this division is…

Earth and Planetary Astrophysics · Physics 2019-09-25 Alexia Simon , Karin I. Oberg , Mahesh Rajappan , Pavlo Maksiutenko

(Abridged) A new type of self-similar hot viscous radiative accretion flow onto a rapidly spinning neutron star has recently been discovered. This ``hot brake'' flow forms in the two-temperature zone (close to a central object), but at a…

Astrophysics · Physics 2007-05-23 Mikhail V. Medvedev

Recent experimental results on the formation of molecular hydrogen on astrophysically relevant surfaces under conditions similar to those encountered in the interstellar medium provided useful quantitative information about these processes.…

Astrophysics · Physics 2009-10-31 Ofer Biham , Itay Furman , Valerio Pirronello , Gianfranco Vidali

H$_2$O$_2$ is part of Europa's water-ice radiolytic cycle and a potential source of oxidants to Europa's subsurface ocean. However, factors controlling the concentration of this critical surface species remain unclear. Though laboratory…

Earth and Planetary Astrophysics · Physics 2024-10-10 Peiyu Wu , Samantha K. Trumbo , Michael E. Brown , Katherine de Kleer

We propose a model describing $N$ spin-1/2 systems coupled through $N$-order homogeneous interaction terms, in presence of local time-dependent magnetic fields. This model can be experimentally implemented with current technologies in…

Quantum Physics · Physics 2018-10-25 R. Grimaudo , L. Lamata , E. Solano , A. Messina

In a recent paper [A. Santos, G. M. Kremer, and V. Garz\'o, \emph{Prog. Theor. Phys. Suppl.} \textbf{184}, 31-48 (2010)] the collisional energy production rates associated with the translational and rotational granular temperatures in a…

Soft Condensed Matter · Physics 2014-11-10 Andrés Santos
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