نتایج جستجو برای: cosmic equilibrium

تعداد نتایج: 160876  

حسین پور, احمد, زارعی, مسلم, قاضی عسگر, سپیده,

The measurement of the polarization of cosmic microwave background (CMB) provides considerable useful information about different physical phenomena at the last scattering surface. The polarization of CMB is due to Compton scattering. In this work, we consider the parity violation of Compton scattering. Then we insert the new amplitude into the quantum Boltzmann equation and show that the forwa...

2008
R. Papoular

It is generally considered, as a rule of thumb, that carbon monoxide forms very early in envelopes of AGB stars, and that it consumes most of the carbon, or most of the oxygen, depending on whether the photosphere is oxygen-rich or carbon-rich, respectively. This work focuses on the latter case , with the purpose of quantifying the remaining fraction of gaseous carbon which is then available fo...

1996
F Combes D Pfenniger

We have recently proposed a new candidate for baryonic dark matter: very cold molecular gas, in near-isothermal equilibrium with the cosmic background radiation at 2.73 K. The cold gas, of quasi-primordial abundances, is condensed in a fractal structure, resembling the hierarchical structure of the detected interstellar medium. We present some perspectives of detecting this very cold gas, eithe...

1999
T. A. Enßlin

We investigate the possibility that patches of old radio plasma ('radio ghosts') of former radio galaxies form a second distinct phase of the inter-galactic medium (IGM), not mixed with the thermal gas. The separation of this phase from the ambient gas and its resistance against eroding turbulent forces is given by magnetic fields, which are expected to be roughly in pressure equilibrium with t...

1997
G. F. Smoot D. Scott

The observed cosmic microwave background (CMB) radiation provides strong evidence for the hot big bang. The success of pri-mordial nucleosynthesis calculations (see Sec. 16, " Big-bang nucle-osynthesis ") requires a cosmic background radiation (CBR) characterized by a temperature kT ∼ 1 MeV at a redshift of z ≃ 10 9. In their pioneering work, Gamow, Alpher, and Herman [1] realized this and pred...

1999
G. E. Allen R. Petre E. V. Gotthelf J. W. Keohane

We present the RXTE PCA X-ray spectrum of SN 1006. This data exhibits evidence of highenergy non-thermal X-ray emission. An analysis of the RXTE PCA data and data from the ASCA SIS and ROSAT PSPC detectors suggests that the entire broad-band X-ray spectrum of SN 1006 may be t with a single non-equilibrium ionization thermal component and a nonthermal component described by a broken power law wi...

Journal: : 2022

If the multiple dualities in Antigone are considered an intragenerational context, i.e. as concordant conflicts Antigone's lifetime, then plot of drama might be perceived stochastic and rather unpredictable to its catastrophic outcome, destruction all protagonists, while their polis is entrapped a seemingly unstable equilibrium. But if viewed transgenerational final episode chain dramatic inter...

2009
R. MEWALDT R. E. VOGT

We report new high resolution measurements of the elemental and isotopic composition of galactic cosmic ray B, C, N, and 0 nuclei with ~ 30 to ~ 130 MeV nucleon-•. These observations place limits on the isotopic composition of the cosmic ray source and restrict possible models of cosmic ray origin and propagation. In particular, we find that N is significantly depleted in the cosmic ray source ...

Journal: :Physical Review D 1994

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