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Tarhan, İsmail

doi:10.1002/1521-3994(200210)323:5<494::aid-asna494>3.0.co;2-e

Cited by 2 publications

(2 citation statements)

References 13 publications

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“…Only if your German diction is that of the elder author. Tarhan (2002) mentions the inclusion of shear and rotation, however, which ought to make the process easier.…”

Section: Their Worlds and Welcome To Themmentioning

confidence: 99%

Astrophysics in 2003

Trimble

Aschwanden

2004

PUBL ASTRON SOC PAC

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Five coherent sections appear this year, addressing solar physics, cosmology (with WMAP highlights), gamma-ray bursters (and their association with Type Ia supernovae), extra-solar-system planets, and the formation and evolution of galaxies (from reionization to assemblage of Local Group galaxies). There are also eight incoherent sections that deal with other topics in stellar, galactic, and planetary astronomy and the people who study them. INTRODUCTIONSTriskaidekaphobics may prefer not to read this installment of ApXX, and their numbers may well be augmented even before the introduction is over. This is, in fact, the 13th overview of 365.24 days of the astronomy and astrophysics literature. The earlier ones are cited here as Ap91, Ap92, …, Ap02 and appear in volumes 104-115 of PASP. The authors have tried to read systematically the contents of about 30 journals and other periodicals. Only about 10% of what has been read gets cited, and being cited is not always an unqualified compliment.Section 2 was assembled using papers found on the Astrophysics Data Service, maintained with support from NASA and including Solar

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“…Only if your German diction is that of the elder author. Tarhan (2002) mentions the inclusion of shear and rotation, however, which ought to make the process easier.…”

Section: Their Worlds and Welcome To Themmentioning

confidence: 99%

Astrophysics in 2003

Trimble

Aschwanden

2004

PUBL ASTRON SOC PAC

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“…In 2003 Mohanty et al [14] studied LRS Bianchi I type universe with attractive massive scalar field in the case of source density model and they have showed that how the dynamical importance of the scalar field and shear change in the course of evolution [14]. Particle physics and high energy astrophysical observations show that the universe is rotating [16][17][18][19][20][21]. A rotating universe with vanishing expansion and shear appeared with the advent of Gödel's universe [20,22].…”

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confidence: 99%

The Decay of Massive Scalar Field in Non-Static Gödel Type Universe with Viscous Fluid and Heat Flow

Aygün

Tarhan

2008

Int J Theor Phys

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In this study, we have investigated the dynamics of non-static Gödel type rotating universe with massive scalar field, viscous fluid and heat flow in the presence of cosmological constant. For various cosmic matter forms, the behavior of the cosmological constant ( ), shear (η) and bulk (ξ ) viscosity coefficients and other kinematic quantities have studied in the early universe. We have showed the decay of massive scalar field in the non-static rotating Gödel type universe and we have obtained constant scalar field with and without source density. Also, we have investigated the effects of massive scalar field on the matter density and pressure. From solutions of the field equations, we have a cosmological model with non-zero expansion, shear, heat flux and rotation. Also some physical and geometrical aspects of the model discussed.

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Untitled

Cited by 2 publications

References 13 publications

Astrophysics in 2003

Astrophysics in 2003

The Decay of Massive Scalar Field in Non-Static Gödel Type Universe with Viscous Fluid and Heat Flow

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