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Dark Matter as Point-like Singularities: Alternative to Dark Halo Model
Dino Martinez1
Section:Survey Paper, Product Type: Journal-Paper
Vol.8 ,
Issue.3 , pp.41-47, Jun-2020
CrossRef-DOI: https://doi.org/10.26438/ijsrpas/v8i3.4147
Online published on Jun 30, 2020
Copyright © Dino Martinez . This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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IEEE Style Citation: Dino Martinez, “Dark Matter as Point-like Singularities: Alternative to Dark Halo Model,” International Journal of Scientific Research in Physics and Applied Sciences, Vol.8, Issue.3, pp.41-47, 2020.
MLA Style Citation: Dino Martinez "Dark Matter as Point-like Singularities: Alternative to Dark Halo Model." International Journal of Scientific Research in Physics and Applied Sciences 8.3 (2020): 41-47.
APA Style Citation: Dino Martinez, (2020). Dark Matter as Point-like Singularities: Alternative to Dark Halo Model. International Journal of Scientific Research in Physics and Applied Sciences, 8(3), 41-47.
BibTex Style Citation:
@article{Martinez_2020,
author = {Dino Martinez},
title = {Dark Matter as Point-like Singularities: Alternative to Dark Halo Model},
journal = {International Journal of Scientific Research in Physics and Applied Sciences},
issue_date = {6 2020},
volume = {8},
Issue = {3},
month = {6},
year = {2020},
issn = {2347-2693},
pages = {41-47},
url = {https://www.isroset.org/journal/IJSRPAS/full_paper_view.php?paper_id=1910},
doi = {https://doi.org/10.26438/ijcse/v8i3.4147}
publisher = {IJCSE, Indore, INDIA},
}
RIS Style Citation:
TY - JOUR
DO = {https://doi.org/10.26438/ijcse/v8i3.4147}
UR - https://www.isroset.org/journal/IJSRPAS/full_paper_view.php?paper_id=1910
TI - Dark Matter as Point-like Singularities: Alternative to Dark Halo Model
T2 - International Journal of Scientific Research in Physics and Applied Sciences
AU - Dino Martinez
PY - 2020
DA - 2020/06/30
PB - IJCSE, Indore, INDIA
SP - 41-47
IS - 3
VL - 8
SN - 2347-2693
ER -
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Abstract :
Observed galactic rotational curves have led to the inference of dark matter. The dark matter halo model is the most prevalent model to this day. This paper introduces an alternative model where dark matter is instead concentrated into massive singularities within galactic clusters. Three different hypothetical cases using this model will be presented here which will simulate rotational curves reminiscent of what has been observed in the study of dark matter. In these different cases, three different positions of a galactic plane orbiting a DM singularity will be modeled to show how the DM has influence on the rotation curves from when the DM singularity is over the center of the galactic plane, to the apsis, and consequently to any position in the orbit. This paper serves as an introduction to this model and a possible new direction in the study of dark matter.
Key-Words / Index Term :
Dark Matter, Dark Matter Halo, Dark Halo Model Alternative, Dark Matter Singularity
References :
[1] van Albada TS, Bahcall JN, Begeman K, and Sancisi R., ?Distribution of dark matter in the spiral galaxy NGC 3198?, The Astrophysical Joutnal, Vol.295, pp.305-313, 1985
[2] Lewis AD, Buote DA, Stocke JT, ?Chandra Observations of A2029: The Dark Matter Profile Down to below 0.01rvir in an Unusually Relaxed Cluster", The Astrophysical Joutnal, Vol.586, No.1, pp.135-142, 2003
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