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Related papers: On the O II ground configuration energy levels

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We consider a gas of bosons interacting through a hard-sphere potential with radius $\frak{a}$ in the thermodynamic limit. We derive a simple upper bound for the ground state energy per particle at low density. Our bound captures the…

Only a few weakly-bound complexes containing the O2 molecule have been characterized by high resolution spectroscopy, no doubt due to the complications added by the oxygen molecule's unpaired electron spin. Here we report an extensive…

Atomic and Molecular Clusters · Physics 2018-07-04 A. J. Barclay , A. R. W. McKellar , N. Moazzen-Ahmadi , Richard Dawes , Xiao-Gang Wang , Tucker Carrington

Planetary Nebulae (PNe) abundance patterns have long been used to note signatures of nuclear processing and to trace the distribution of metals throughout galaxies. We present abundance gradients and heavy element ratios based upon newly…

Astrophysics · Physics 2009-11-11 J. B. Milingo , K. B. Kwitter , R. B. C. Henry , S. P. Souza

Planetary nebulae (and in general any photoionized region) can be classified as ionization-bounded or density-bounded. It is important to determine in which case is the planetary nebula studied to be able to estimate from nebular…

Astrophysics of Galaxies · Physics 2009-02-23 L. F. Rodriguez , Y. Gomez , L. Guzman

NASA's Habitable Worlds Observatory (HWO) will search for biosignatures on Earth-like exoplanets using reflected light spectroscopy. A critical instrument design parameter is resolving power, which must balance biosignature detectability…

Earth and Planetary Astrophysics · Physics 2026-04-30 Samantha Gilbert-Janizek , Jacob Lustig-Yaeger , Joshua Krissansen-Totton

We present BOND, a Bayesian code to simultaneously derive oxygen and nitrogen abundances in giant H II regions. It compares observed emission lines to a grid of photoionization models without assuming any relation between O/H and N/O. Our…

Astrophysics of Galaxies · Physics 2016-05-05 N. Vale Asari , G. Stasińska , C. Morisset , R. Cid Fernandes

The atmospheric composition of transiting exoplanets can be characterized during transit by spectroscopy. For the transit of an Earth twin, models predict that biogenic $O_2$ and $O_3$ should be detectable, as well as water vapour, a…

We are engaged in a comprehensive program to find reliable elemental abundances in and to probe the physical structure of the Orion Nebula, the brightest and best-resolved H II region. In the course of developing a robust extinction…

We present spectrophotometry in the 3600-9700 A region for a sample of 39 H II regions in the Galaxy and Magellanic Clouds, for which independent information is available on the spectral types and effective temperatures of the ionizing…

Astrophysics · Physics 2019-08-17 R. C. Kennicutt, , F. Bresolin , H. French , P. Martin

We describe a numerical study of the potential energy landscape for the two-dimensional XY model (with no disorder), considering up to 100 spins and CPU and GPU implementations of local optimization, focusing on minima and saddles of index…

Statistical Mechanics · Physics 2013-11-27 Dhagash Mehta , Ciaran Hughes , Mario Schröck , David J. Wales

Extensive variational computations are reported for the ground state energy of the non-relativistic two-electron atom. Several different sets of basis functions were systematically explored, starting with the original scheme of Hylleraas.…

Atomic Physics · Physics 2009-11-07 Charles Schwartz

Energy levels, Land\'{e} $g$-factors and radiative lifetimes are reported for the lowest 182 levels of the 3d$^4$, 3d$^3$4s and 3d$^3$4p configurations of Fe~V, Co~VI and Ni~VII. Additionally, radiative rates ($A$-values) have been…

Atomic Physics · Physics 2017-03-08 K. M. Aggarwal , P. Bogdanovich , F. P. Keenan , R. Kisielius

Spectrophotometry constitutes a unique way to obtain the whole diagnostics (density, temperature, ionic abundances) of ionized gas nebulae, thus providing invaluable information about the objects where they reside. If such nebulae are in…

Astrophysics · Physics 2007-05-23 E. Perez-Montero , A. I. Diaz

Using density functional theory implemented within the generalized gradient approximation, a new non-magnetic insulating ground state of solid oxygen is proposed and found to be energetically favored at pressures corresponding to the…

Materials Science · Physics 2009-11-07 J. B. Neaton , N. W. Ashcroft

We present here a formulation of the electronic ground-state energy in terms of the second order reduced density matrix, using a duality argument. It is shown that the computation of the ground-state energy reduces to the search of the…

Quantum Physics · Physics 2009-11-13 Eric Cances , Gabriel Stoltz , Mathieu Lewin

In the last decade ground based high resolution Doppler spectroscopy (HRS) has detected numerous species in transiting and non-transiting hot Jupiters, and is ideally placed for atmospheric characterisation of warm Neptunes and super…

Earth and Planetary Astrophysics · Physics 2020-09-09 Siddharth Gandhi , Matteo Brogi , Rebecca K. Webb

Based on high quality observations of multiplet V1 of OII and the NLTE atomic computations for OII we study the density and temperature of a sample of PNe. We find that, in general, the densities derived from recombination lines of OII are…

Astrophysics of Galaxies · Physics 2014-08-22 Antonio Peimbert , Manuel Peimbert , Gloria Delgado-Inglada , Jorge Garcia-Rojas , Miriam Peña

The isotropic scattering phase shift is calculated for non-relativistic bosons interacting at low energies via an arbitrary finite-range potential in d spacetime dimensions. Scattering on a (d-1)-dimensional torus is then considered, and…

Quantum Gases · Physics 2011-04-14 Silas R. Beane

We derive an approximate analytic formula for the ground-state energy of the charged anyon gas. Our approach is based on the harmonically confined two-dimensional (2D) Coulomb anyon gas and a regularization procedure for vanishing…

Strongly Correlated Electrons · Physics 2009-11-13 B. Abdullaev , U. Roessler , M. Musakhanov

The carbon dimer, the $^{12}$C$_2$ molecule, is ubiquitous in astronomical environments. Experimental-quality rovibronic energy levels are reported for $^{12}$C$_2$, based on rovibronic transitions measured for and among its singlet,…

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