Neutron Stars Accreting Matter and A Wave Model

Physics

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In 1990 I proposed that oscillating stars and planets radiate quantum like standing waves providing for the spacings of planets and satellites. Waves also provide stability for star systems and the universe (see Physics Essays 12(1): 3-10 for a wave equation and solutions). Radii of orbits are given by r=R(exp(kN)) where R is the radius of the star and N is the orbit integer. k is 0.625 for matter free regions apparently becoming less depending on the density of matter present. This equation or similar may provide an incredibly simple explanation of the most often observed QPO's of matter accreting neutron stars if one assumes that the highest amplitude, highest frequency QPO is due to the N=2 orbit. Since incredibly large gravitational fields are involved the equation may be different. In the usual model a second weaker observed lower frequency QPO is explained as the beat frequency of the star spin frequency with the large amplitude QPO. High density neutron stars likely provide particularly strong orbital forces constraining the accreting matter. See the Wagner web site.

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