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Crystallography 2018
Structural Chemistry & Crystallography Communication
ISSN: 2470-9905
Page 56
June 04-05, 2018
London, UK
3
rd
Edition of International Conference on
Advanced Spectroscopy,
Crystallography and Applications
in Modern Chemistry
T
he x-ray femtoscope measures dimensions and interactions
in the range of femtometers. In this way it detects interactions
at the boundary of the nuclear surface, and has even allowed
measuring the radii of protons on the nuclear surface and the
electrons of the K layer [1], [2]. To measure dimensions of the
order of the femtometers, it uses resonance and interference of
the x-rays with the nuclear surface, using only the K edge data, for
each of the elements of the periodic table 11 <Z <92. Because of
the non-invasive nature of low energy x-rays, we can measure a
minimal abnormality of the cross section or energy (k edge) on
the nuclear surface. For this reason, we can detect dark matter
or WIMPs, which interact and hide on the nuclear surface [3].
Fortunately, after studying these interactions with all the elements
of the periodic table, only three elements: Cr, Xe and Tm present
resonances. Dark matter (< (100±2) eV/c²) acts directly and
resonantly with the excess mass, energy and cross section of the
atomic nuclei of xenon, thulium and chromium, through the weak
force, which is represented by the solution of the Navier Stokes
equations [4].Thedarkmatter ishidden in thevicinityof thenuclear
surface (10⁻¹⁸m), it interacts modifying the effective sections and
the K edge energy [5]. We studied the total absorption of low
energy x-rays (<1.16MeV) for the elements of the periodic table
11≤Z≤90, with a precision of the order of the Rydberg constant,
and the radius of the neutron (0.842 (3) fm) using experimental
NIST data and GEANT4 simulation for (0.993(9) <R²<0.999(6))
[6]. Finally, it was proved theoretically and experimentally that the
weak force controls the circular trajectories of the nucleon layers
in the atomic nucleus, the interaction with dark matter and the
nuclear stability P (x, y, z)..
Figure 1. A:
Cross section excess measure presence of dark matter for
24Cr and 69Tm. B.-Evolution of nuclear stability P, depending on the ratio
of the cross sections. We obtained the probability P (x, y, z, t) which is the
fundamental solution of the Navier Stokes equations, measures the Nuclear
stability and represents both the behavior of the atomic nucleus in equilib-
rium and out of equilibrium such us gamma or beta decay C.- Calculation
of the Rydberg constant using Navier Stokes model. D.- Energy excess. For
54Xe, we can see the resonance in energy.
Recent Publications
1. Jimenez, Recalde, Jimenez Chacon (2017). Extraction of
the Proton and Electron Radii fromCharacteristic Atomic
Lines and Entropy Principles. Entropy 2017.
2. Pohl, R et al. (2010). The size of the proton. Nature 2010,
466, 213--216.
3. M. Markevitch, A. H. Gonzalez, D. Clowe et al (2004) :
DIRECT CONSTRAINTS ON THE DARK MATTER SELF-
INTERACTION CROSS SECTION FROM THE. MERGING
GALAXY CLUSTER 1E 0657 56. The Astrophysical
Journal, 606:819--824, (2004).
4. David Harvey F. Courbin J. P. Kneib et al. (2017) : A
detection of wobbling brightest cluster galaxies within
massive galaxy clusters. Monthly Notices of the Royal
Astronomical Society, Volume 472, Issue 2, 1 December
2017.
5. Masahiro Kawasaki, Kazunori Kohri and Takeo Moroi
(2018): Revisiting big-bang nucleosynthesis constraints
on long-lived decaying particles, PHYSICAL REVIEW D
97, 023502 (2018)
6. E. Aprile et al. (2017) : Search for bosonic super-WIMP
interactions with the XENON100 experiment,. (XENON
Collaboration), Phys. Rev. D 96, 122002, (2017).
THE X-RAY FEMTOSCOPE ALLOWS US TO MEASURE THE INTERACTION
BETWEEN DARK MATTER AND THE ATOMIC NUCLEI OF CR, XU AND TM
Edward Jimenez
Central University, Ecuador
Edward Jimenez, Struct Chem Crystallogr Commun 2018, Volume 4
DOI: 10.21767/2470-9905-C1-006