Solution of Einsteinas Field Equations for Mixed Potential of a Radiating Star

1
Dr. M. A. Helal
Dr. M. A. Helal
2
M. M. R. Chowdhury
M. M. R. Chowdhury
3
M. K. H. Chowdury
M. K. H. Chowdury
4
M. A. Islam
M. A. Islam
1 University of Chittagong, Chittagong, Bangladesh.

Send Message

To: Author

GJSFR Volume 12 Issue F9

Article Fingerprint

ReserarchID

O0EDM

Solution of Einsteinas Field Equations for Mixed Potential of a Radiating Star Banner
  • English
  • Afrikaans
  • Albanian
  • Amharic
  • Arabic
  • Armenian
  • Azerbaijani
  • Basque
  • Belarusian
  • Bengali
  • Bosnian
  • Bulgarian
  • Catalan
  • Cebuano
  • Chichewa
  • Chinese (Simplified)
  • Chinese (Traditional)
  • Corsican
  • Croatian
  • Czech
  • Danish
  • Dutch
  • Esperanto
  • Estonian
  • Filipino
  • Finnish
  • French
  • Frisian
  • Galician
  • Georgian
  • German
  • Greek
  • Gujarati
  • Haitian Creole
  • Hausa
  • Hawaiian
  • Hebrew
  • Hindi
  • Hmong
  • Hungarian
  • Icelandic
  • Igbo
  • Indonesian
  • Irish
  • Italian
  • Japanese
  • Javanese
  • Kannada
  • Kazakh
  • Khmer
  • Korean
  • Kurdish (Kurmanji)
  • Kyrgyz
  • Lao
  • Latin
  • Latvian
  • Lithuanian
  • Luxembourgish
  • Macedonian
  • Malagasy
  • Malay
  • Malayalam
  • Maltese
  • Maori
  • Marathi
  • Mongolian
  • Myanmar (Burmese)
  • Nepali
  • Norwegian
  • Pashto
  • Persian
  • Polish
  • Portuguese
  • Punjabi
  • Romanian
  • Russian
  • Samoan
  • Scots Gaelic
  • Serbian
  • Sesotho
  • Shona
  • Sindhi
  • Sinhala
  • Slovak
  • Slovenian
  • Somali
  • Spanish
  • Sundanese
  • Swahili
  • Swedish
  • Tajik
  • Tamil
  • Telugu
  • Thai
  • Turkish
  • Ukrainian
  • Urdu
  • Uzbek
  • Vietnamese
  • Welsh
  • Xhosa
  • Yiddish
  • Yoruba
  • Zulu

We have studied the behaviour of a radiating star when the interior expanding, shearing fluid particles are traveling in geodesic motion. A systematic approach enables us to write the junction condition as a Riccati equation. In this article we obtained two new solutions in terms of elementary functions with assuming a separation of variables and also have discussed the physical significance of these solutions.

7 Cites in Articles

References

  1. A De Oliviera,N Santos,C Kolassis (1985). Collapse of a Radiating Star.
  2. L Herrera,G Le Denmat,N Santos,A Wang (2004). Shear-free Radiating Collapse & Conformal Flatness.
  3. L Herrera,A Di Prisco,J Ospino (2005). Some analytical models of radiating collapsing spheres.
  4. N Naidu,M Govender,K Govinder (2006). THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR.
  5. S Rajah,S Maharaj (2008). A Riccati Equation in Radiative Stellar Collapse.
  6. P Nogueira,R Chan (2004). RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR VISCOSITY AND BULK VISCOSITY.
  7. S Thirukkanesh,S Maharaj (2010). Mixed potentials in radiative stellar collapse.

Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

Ethical Approval

No ethics committee approval was required for this article type.

Data Availability

Not applicable for this article.

Dr. M. A. Helal. 2012. \u201cSolution of Einsteinas Field Equations for Mixed Potential of a Radiating Star\u201d. Global Journal of Science Frontier Research - F: Mathematics & Decision GJSFR-F Volume 12 (GJSFR Volume 12 Issue F9): .

Download Citation

Issue Cover
GJSFR Volume 12 Issue F9
Pg. 13- 19
Journal Specifications

Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

Classification
Not Found
Version of record

v1.2

Issue date

August 7, 2012

Language

English

Experiance in AR

The methods for personal identification and authentication are no exception.

Read in 3D

The methods for personal identification and authentication are no exception.

Article Matrices
Total Views: 5004
Total Downloads: 2492
2026 Trends
Research Identity (RIN)
Related Research

Published Article

We have studied the behaviour of a radiating star when the interior expanding, shearing fluid particles are traveling in geodesic motion. A systematic approach enables us to write the junction condition as a Riccati equation. In this article we obtained two new solutions in terms of elementary functions with assuming a separation of variables and also have discussed the physical significance of these solutions.

Our website is actively being updated, and changes may occur frequently. Please clear your browser cache if needed. For feedback or error reporting, please email [email protected]
×

This Page is Under Development

We are currently updating this article page for a better experience.

Request Access

Please fill out the form below to request access to this research paper. Your request will be reviewed by the editorial or author team.
X

Quote and Order Details

Contact Person

Invoice Address

Notes or Comments

This is the heading

Lorem ipsum dolor sit amet, consectetur adipiscing elit. Ut elit tellus, luctus nec ullamcorper mattis, pulvinar dapibus leo.

High-quality academic research articles on global topics and journals.

Solution of Einsteinas Field Equations for Mixed Potential of a Radiating Star

Dr. M. A. Helal
Dr. M. A. Helal University of Chittagong, Chittagong, Bangladesh.
M. M. R. Chowdhury
M. M. R. Chowdhury
M. K. H. Chowdury
M. K. H. Chowdury
M. A. Islam
M. A. Islam

Research Journals