Abstract
Neutron stars (NS) are one of the probable signals of early universe formation in which the quark and gluons are defined in free degree of freedom. Like NS a boson Star (BS) is formed out of particles called bosons. For the existence of stars, there must be a stable type of boson that possesses a small mass of magnitude. Such systems must be formed by perturbation of small potential under the weak gravity limit.These pattern are shown by the oscillations of BS.
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Acknowledgements
I am very much thankful to Dr.Naimuddin, faculty, University of Delhi, Delhi-7, for his support in publishing the manuscript in this reputed journal series. I thank University of Delhi, Delhi-110007 for providing the R and D research grant, 2016 as financial support.
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Jarwal, B., Singh, S.S. (2018). Rotating Boson Star Under Weak Gravity Potential. In: Naimuddin, M. (eds) XXII DAE High Energy Physics Symposium . Springer Proceedings in Physics, vol 203. Springer, Cham. https://doi.org/10.1007/978-3-319-73171-1_190
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DOI: https://doi.org/10.1007/978-3-319-73171-1_190
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