We present Dark Matter candidates from non SUSY processes, in a way emphasizing how a Dark Matter (DM) candidate of roughly 100 - 400 GeV could be formed. As has been said about the Photon rocket and Axions rockets, the presence of a magnetic field supposedly would switch DM particle candidates to photons, in such a way as to in the end configure a photon rocket style device from DM in a thrust chamber. The presence of Dark Matter (DM) would in itself merely indicate that the emerging photon thrust would be comparatively greater than it would be for more conventional photon rockets. This amplifies and improves upon a so called axion rocket ram jet for interstellar travel. We assume that much the same sort of methodology for a would-be axion ramjet could be employed for DM, with perhaps greater thrust/power conversion efficiencies.
References
[1]
Beckwith, A.W. (2008) The Author Gave Substantially This Presentation in Stockholm, Sweden, in IDM. http://agenda.albanova.se/confRegistrantsDisplay.py/list?confId=355
[2]
Hooper, D. (2008) http://agenda.albanova.se/confRegistrantsDisplay.py/list?confId=355
[3]
Hooper, D. and Goodenough, L. (2011) Dark Matter Annihilation in the Galactic Center as Seen by the Fermi Gamma Ray Space Telescope. Physics Letters B, 697, 412-428.
http://arxiv.org/abs/1010.2752v3
http://dx.doi.org/10.1016/j.physletb.2011.02.029
[4]
Meissner, K. and Nicolai, H. (2007) Conformal Symmetry and the Standard Model. Physics Letters B, 648, 312-317. https://arxiv.org/abs/hep-th/0612165
http://dx.doi.org/10.1016/j.physletb.2007.03.023
[5]
Drewes, M. (2013) The Phenomenology of Right Handed Neutrinos. International Journal of Modern Physics E, 22, 1330019. https://arxiv.org/abs/1303.6912
http://dx.doi.org/10.1142/s0218301313300191
[6]
Lemos, R. (2008) Scientists Say We Will Never Reach the Stars. Wired Magazine (August).
http://www.wired.com/science/space/news/2008/08/space_limits
Beckwith, A.W. (2009) Hypothetical Dark Matter/Axion Rockets: What Can Be Said about Dark Matter in Terms of Space Physics Propulsion. Contributed to SPESIF-2009, Huntsville, 24-27 February 2009. http://arxiv.org/abs/0810.1493
http://dx.doi.org/10.1063/1.3115506
[9]
Corda, C. (2009) Interferometric Detection of Gravitational Waves: The Definitive Test for General Relativity. International Journal of Modern Physics D, 18, 2275.
https://arxiv.org/abs/0905.2502
http://dx.doi.org/10.1142/S0218271809015904
[10]
Nojiri, S. and Odintsov, S. (2011) Unified Cosmic History in Modified Gravity: From F(R) Theory to Lorentz Non-Invariant Models. Physics Reports, 505, 59.
http://arxiv.org/pdf/1011.0544.pdf
http://dx.doi.org/10.1016/j.physrep.2011.04.001
[11]
Collar, J.I., Miller, D., Rasmussen, J., et al. (2005) CAST, The Solar Axion Search at CERN.
http://collargroup.uchicago.edu/projects/axion/index.html
[12]
Yang, Q. (2015) Axions and Dark Matter. https://arxiv.org/abs/1509.00673
[13]
Kolb, E., Pi, S.-Y. and Raby, S. (1984) Phase Transitions in Supersymmetric Grand Unified Models. In: Fang, L.Z. and Ruffini, R., Eds., Cosmology of the Early Universe, World Press Scientific.
[14]
Kolb, E.W. and Turner, M.S. (1990) The Early Universe. Addison-Wesley Publishing Company, The Advanced Book Program, Redwood City.
[15]
Muramaya, H. (2006) Physics beyond the Standard Model and Dark Matter. Session LXXXVI of Les Houches.
Blandford, R.D. and Narayan, R. (1992) Cosmological Applications of Gravitational Lensing. Annual Review of Astronomy and Astrophysics, 30, 311-358.
[18]
Roland, S. (2015) A New Model for Sterile Neutrino Dark Matter.
https://indico.cern.ch/event/373156/contributions/1793073/attachments/1142692/1637250/New_ Neutrino_DM_Model.pdf
[19]
Madsen, J. (1991) Generalized Tremaine-Gunn Limits for Bosons and Fermions. Physical Review D: Particles and Fields, 44, 999-1006. http://dx.doi.org/10.1103/PhysRevD.44.999
[20]
Peebles, P.J.E. (1993) Principles of Physical Cosmology. Princeton Series in Physics.
[21]
Adhikari, R., et al., Including Ruchayskiy, O. (2016) A White Paper on keV Sterile Neutrino Dark Matter. http://arxiv.org/abs/1602.04816
[22]
Taoso, M., Bertone, G. and Masiero, A. (2008) Dark Matter Candidates: A Ten-Point Test. JCAP 0803:022,2008. https://arxiv.org/abs/0711.4996
[23]
Gulevich, A., Ivanov, E., Kukharchuk, O., Poupko, V.Y. and Zrodnikov, A.V. (2001) Applications of Nuclear Photon Engines for Deep Space Exploration. AIP Conference Proceedings, 552, 957-962. http://dx.doi.org/10.1063/1.1358034
[24]
Sikivie, P. (1983) Experimental Tests of the “Invisible” Axion. Physical Review Letters, 51, 1415. http://dx.doi.org/10.1103/PhysRevLett.51.1415
[25]
Rizzo, C., Sautivet, A.-M., et al. (2007) No Light Shining through a Wall. CRNS: France, arXiv. http://arxiv.org/pdf/0707.1296
[26]
Ruchayskiy, O. (2007) Restrictions on Sterile Neutrino Parameters from Astrophysical Observations. ArXiv 0704.3215v1.