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Related papers: Electron temperature fluctuations in Seyfert galax…

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We report on very low temperature (27 mK) Mossbauer absorption spectra on Gd 155 in the Heisenberg frustrated antiferromagnets Gd2 Sn2 O7 (GdSn) and Gd2 Ti2 O7. We show that electronic fluctuations of correlated Gd3+ moments are present…

Condensed Matter · Physics 2009-11-07 E. Bertin , J. A. Hodges , J. -P. Bouchaud , P. Bonville , J. P. Sanchez , P. Vuillet

We propose a method of measuring the electron temperature $T_e$ in mesoscopic conductors and demonstrate experimentally its applicability to micron-size graphene devices in the linear-response regime ($T_e\approx T$, the bath temperature).…

Mesoscale and Nanoscale Physics · Physics 2009-04-29 K. Kechedzhi , D. W. Horsell , F. V. Tikhonenko , A. K. Savchenko , R. V. Gorbachev , I. V. Lerner , V. I. Fal'ko

We describe here a minimal theory of tight binding electrons moving on the square planar Cu lattice of the hole-doped cuprates and mixed quantum mechanically with pairs of them (Cooper pairs). Superconductivity occurring at the transition…

Strongly Correlated Electrons · Physics 2013-05-29 Sumilan Banerjee , T V Ramakrishnan , C Dasgupta

A present prevailing open problem planetary nebulae research, and photoionized gaseous nebulae research at large, is the systematic discrepancies in ionic abundances derived from recombination and collisionally excited lines in many H II…

Solar and Stellar Astrophysics · Physics 2017-09-26 Manuel A. Bautista , Ehab E. Ahmed

We investigate the electron temperature gradient in the galactic disk as measured by young HII regions on the basis of radio recombination lines and the corresponding gradient in planetary nebulae (PN) based on [OIII] electron temperatures.…

Astrophysics · Physics 2015-06-24 W. J. Maciel , C. Quireza , R. D. D. Costa

A lagrangian for the $k-$ essence field is constructed for a constant scalar potential and its form determined when the scale factor was very small compared to the present epoch but very large compared to the inflationary epoch. This means…

General Relativity and Quantum Cosmology · Physics 2014-11-18 Debashis Gangopadhyay

We present a high spatial resolution map of the columnar electron temperature (Tc) of a region to the south west of the Trapezium in the Orion Nebula. This map was derived from Hubble Space Telescope images that isolated the primary lines…

Astrophysics · Physics 2009-11-07 C. R. O'Dell , M. Peimbert , A. Peimbert

The near-infrared spectra of Active Galactic Nuclei (AGN) present emission lines of different atomic and molecular species. The mechanisms involved in the origin of these emission lines in AGN are still not fully understood. We use J and K…

We present a new model for the Galactic distribution of free electrons. It (a) describes the distribution of the free electrons responsible for pulsar dispersion measures and thus can be used for estimating the distances to pulsars; (b)…

Astrophysics · Physics 2009-09-29 J. M. Cordes , T. J. W. Lazio

We have performed a detailed analysis of the electron temperature and density in the the Ring Nebula using the calibrated HST WFC3 images described in the preceding paper. The electron temperature (Te) determined from [N II] and [O III]…

Astrophysics of Galaxies · Physics 2016-11-04 C. R. O'Dell , G. J. Ferland , W. J. Henney , Manuel Peimbert

The presence of convective and turbulent motions, and the evolution of magnetic fields give rise to existence of temperature fluctuations in stellar atmospheres, active galactic nuclei and other cosmic objects. We observe the time and…

Solar and Stellar Astrophysics · Physics 2015-06-04 N. A. Silant'ev , G. A. Alekseeva , V. V. Novikov

We calculate suppression of inter- and intralayer superconducting currents due to equilibrium phase fluctuations and find that, in contrast to a recent prediction, the effect of thermal fluctuations cannot account for linear temperature…

Superconductivity · Physics 2009-10-31 S. N. Artemenko , S. V. Remizov

Electron temperatures derived from the \ion{He}{1} recombination line ratios, designated $T_{\rm e}$(\ion{He}{1}), are presented for 48 planetary nebulae (PNe). We study the effect that temperature fluctuations inside nebulae have on the…

Astrophysics · Physics 2009-11-10 Y. Zhang , X. -W. Liu , Y. Liu , R. H. Rubin

We present HST/STIS long-slit spectroscopy of NGC 1976. Our goal is to measure the intrinsic line ratio [O III] 4364/5008 and thereby evaluate the electron temperature (T_e) and the fractional mean-square T_e variation (t_A^2) across the…

We present ALMA observations at 233, 678, and 870 GHz of the Galactic Center black hole, Sagittarius A*. These observations reveal a flat spectrum over this frequency range with spectral index $\alpha \approx -0.3$, where the flux density…

In a very recent work, [1] claim that the scenario of temperature inhomogeneities proposed by [2] ($t2$ > 0) is not able to explain the O$^{2+}$/H$^{+}$ abundance discrepancy observed between the calculations based on the optical [OIII]…

Astrophysics of Galaxies · Physics 2023-10-03 J. Eduardo Méndez-Delgado , César Esteban , Jorge García-Rojas , Kathryn Kreckel , Manuel Peimbert

A new thermometer based on fragment momentum fluctuations is presented. This thermometer exhibited residual contamination from the collective motion of the fragments along the beam axis. For this reason, the transverse direction has been…

Contrary to the starting assumption of Grbi\'c et al. (Phys. Rev. B 83, 144508 (2011)), here we will first argue that a 16 T magnetic field is not enough to quench all superconducting fluctuations above Tc in YBa$_2$Cu$_3$O$_{7-\delta}$. We…

Superconductivity · Physics 2021-01-28 D. Sóñora , J. Mosqueira , F. Vidal

We measure the temperature of a mesoscopic system consisting of an ultra-dilute two dimensional electron gas at the $Si/SiO_2$ interface in a metal-oxide-semiconductor field effect transistor (MOSFET) quantum dot by means of the capture and…

Mesoscale and Nanoscale Physics · Physics 2015-05-18 Enrico Prati , Matteo Belli , Marco Fanciulli , Giorgio Ferrari

A novel method to determine the density and temperature of a system is proposed based on quantum fluctuations typical of Fermions in the limit where the reached temperature T is small compared to the Fermi energy $\epsilon_f$ at a given…

Nuclear Theory · Physics 2011-06-27 Hua Zheng , Aldo Bonasera