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Stealth, Invisibility

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Lehnert (2002) presents 10 failures of Maxwell's equations. ... Known greatest length = 100,000 km ... In this example L1% 100,000km (L1% = length when ... – PowerPoint PPT presentation

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Title: Stealth, Invisibility


1
Stealth, Invisibility Deep Space Radiation
Shielding
  • Benjamin T Solomon
  • Interstellar Space Exploration Technology
    Initiative
  • iSETI LLC
  • P.O. Box 831
  • Evergreen, CO 80439
  • benjamin.t.solomon _at_ iseti.us

2
Biography
  • 2010 Session Co-Chairman, A03.1. Theories,
    Models and Concepts at Space, Propulsion
    Energy Sciences International Forum (SPESIF
    2010), Kossiakoff Center, Applied Physics
    Laboratory, Johns Hopkins University
  • 2009 Space Propulsion Energy Sciences
    International Forum, (American Institute of
    Physics Conference Proceeding), gravitational
    acceleration without mass valid for gravity,
    mechanical electromagnetic forces.
  • 2001 Current Numerous presentations papers
    on gravity modification at space conferences.
  • 1999 Inventor of proprietary electrical circuits
    (with no moving parts) that can change weight (
    3 to 5 over 2 hours one 98 loss for about
    a minute). An engine technology without moving
    parts.

g t c2
3
Overview
  • Introduction/Objectives/Approach
  • Non-Gaussian Photon Probability Distribution
  • Shielding, Cloaking Invisibility

4
Introduction
  • Lehnert (2002) presents 10 failures of Maxwells
    equations. Two of these are wave-particle plane
    wave-dot. These 2 phenomenon have not been
    unified.
  • Hunter et al (2002) focused only on the
    electromagnetic soliton wave function (no
    consideration for the photons probabilistic
    properties).
  • Solomon (2009) had shown that gravitational
    acceleration is independent of the internal
    nature of a particle. Could one experimentally
    determine the nature of a particle? This work is
    in it early stages and some equations are quick
    dirty.
  • The probabilistic approach provides an avenue to
    unify shielding, stealth or cloaking
    invisibility without consideration for
    electromagnetic properties.
  • Would like to collaborate with experimenters and
    manufacturers to develop new materials with this
    approach. Seeking funding for this research.

5
Objectives
  • To present a new approach to determining photon
    behavior based on the discovery that the photon
    probability distribution is not a Gaussian
    function and it is huge.

6
Approach
  • Use of numerical modeling to determine the
    probability distribution that best fits the
    experimental data.
  • Separate the probability distribution function
    from the electromagnetic wave function.
  • Determine what types of photon behavior are best
    modeled by the probability distribution itself.

7
Non-Gaussian Photon Probability Distribution
8
The Airy Disc
Rings composed of dots of localizations of the
electromagnetic function. (Photo Source
Wikipedia)
9
Fitting the Distribution
  1. Normal Distribution Tail too short cannot
    explain long tailed intensity dispersion.
  2. Modified Gamma Fits the intensity dispersion
    correctly.
  1. Modified Gamma A function of the space around
    the photon and therefore explains why and how the
    observer alters the observation.

10
Distribution Along Cross-Section
  1. As ??90 the cross-sectional distribution becomes
    Normal
  2. As ??0 the cross-sectional distribution in no
    longer Normal

11
Comparing with Best Fit Normal
? is small
? is large
  1. Cross-Sectional photon probability distribution
    is not a Normal Distribution.
  2. Photon distribution changes shape with angle from
    pinhole.

12
Distribution Along an Arc
  1. The photon probability distribution along an arc
    is not a Normal Distribution.
  2. The photon distribution changes shape with
    distance from pinhole.

13
Distribution Along Axis of Motion
Decreasing r.
  1. Within the limits of sampling intervals the
    probability distribution resembles a Lognormal
    Distribution.
  2. Note that the length of the probability
    distribution is on the order of 1,000s km. In
    this example L1 gt 100,000km (L1 length when
    probability lt 1)

14
The Effect of ?/Da on Length
Increasing ?/DA
Increasing DA
Distribution Lengthens
  1. The length of the probability distribution
    increases as the pinhole size increases.

15
The Effect of ?/Da on Height
Distribution shifts left or shortens
  1. The probability distribution can be spread as
    much as 16m from the axis of motion.
  2. The probability distribution narrows as the
    pinhole size is decreased.
  3. The pinhole size can be used to narrow and
    lengthen the photon probability distribution.
    This is termed the squeezing effect.

16
Photon Probability Shape
17
Additional Restrictions on Entanglement
Experiments
Cannot do entanglement test in this region
gt16m
gt16m
gt16m
gt16m
Photon path
Photon path
Reflection only permitted after test.
Reflection only permitted after test.
gt16m
gt16m
Permitted region for entanglement test.
Permitted region for entanglement test.
18
Additional Restrictions on Entanglement
Experiments
  • Not allowed
  • When 2 photons head towards each other.
  • When the two parallel photons axes of motion are
    less than 32 m apart.
  • Photon path reflection before and during test.
  • If the modified Gamma photon probability is not
    the cause of quantum entanglement, then with
    these restrictions, probability of entangled
    observations gt1.

19
Shielding, Cloaking Invisibility
20
Probabilistic Shielding Hypothesis
Simplified Otoshi
Slot
Prob. Distn.
  1. Shielding Effectiveness, SEP, is defined as the
    ability to stop photon propagation through holes
    of radius r in the material. Or ratio of
    probability outside the hole.
  2. The ability of a photon to pass through an
    aperture of size d is primarily determined by its
    probability function.
  3. Given this probability function, the secondary
    shielding characteristics are the electromagnetic
    function that are overlaid on top of this
    probabilistic function.

21
Comparisons with Experimental Data
Simplified Otoshi
Slot
Prob. Distn.
  1. The Otoshi and Slot functions agree with each
    other.
  2. The probability (in dB) agrees substantially .
  3. Differences due to electromagnetic effects
    undetermined pinhole size, DA.
  4. Can separate probabilistic from electromagnetic
    effects.

Quick Dirty
22
Typical Electromagnetic Component
Electromagnetic effect is non-linear
Electromagnetic effect is linear
  1. The probability hypothesis suggests that for
    aperture sizes gt 0.4 wavelength, the
    electromagnetic effect is linear.
  2. Need to build model of the non-probabilistic
    electromagnetic effects.

23
Probabilistic Cloaking Hypothesis
To counteract cloaking, reduce wavelength to lt
1/91.5x (gt10dB)
Stealth Cloaking
Cloaking is possible if object size is lt 12.5
wavelength (lt1dB)
  1. Cloaking Effectiveness, CEP, is defined ratio of
    the distribution that is present outside the
    obstruction of radius r, i.e. the probability
    distribution that escapes around the disc or
    obstruction.
  2. Using the same parameters as Schurig et al, 2006,
    the probability distribution model shows that if
    disc size lt12.5x wavelength, transmission is
    assured (lt1dB).
  3. However, this model does not describe the
    electromagnetic effects of the material on the
    photon. Material properties are also key to
    cloaking.

24
Probabilistic Invisibility Hypothesis
Obstruction
The quick dirty ?/DA for a required cum prob.
Pgtr (e.g. 1) beyond a radial distance r from
the axis of motion.
  1. Invisibility Effectiveness, IEP, is defined as
    the ability to pass through the spaces between
    atoms and molecules of radius r without
    interacting with the material. The ratio of the
    distribution that pass through the aperture.
  2. This is achieved by squeezing the photon
    probability distribution.
  3. Photon squeezing cannot be achieved by physical
    aperture manipulation alone but requires a
    technological solution.

25
The Future of Materials Design
There are 2 materials design strategies,
shielding or invisibility that can be used for
deep space radiation shielding.
Molecules
Molecules
26
Conclusion
  • Explained how the observer alters the
    observation.
  • Showed that the photon probability distribution
    is non-Gaussian huge.
  • Explained Shielding, Cloaking/Stealth, and
    Invisibility in terms of the new non-Gaussian
    distribution. That these 3 phenomena are
    essentially the same.
  • Identified 2 new strategies for materials design.
  • Seeking collaboration funding.

27
Bibliography
  • Hunte, G., Kowalski, M., Mani, R., Wadlinger,
    R.L.P., Engler, F., Richardson, T. From the
    Hubble Radius to the Plank Scale, Proceedings of
    a Symposium in Honour of the 80th Birthday of
    Jean-Pierre Vigier, Edited by Amoroso, R.L.,
    Hunter, G., Kafatos, M., and Vigier, J-P., Kluwer
    Academic Publishers, Boston, (2002)
  • Lenhert, B.O. New Developments in
    Electromagnetic Theory, From the Hubble Radius
    to the Plank Scale, Proceedings of a Symposium in
    Honour of the 80th Birthday of Jean-Pierre
    Vigier, Edited by Amoroso, R.L., Hunter, G.,
    Kafatos, M., and Vigier, J-P., Kluwer Academic
    Publishers, Boston, (2002).
  • Otoshi, T.Y. A study of microwave transmission
    through perforated flat plates. JPL Technical
    Report, 32-1526, Vol. II (1972).
  • Schurig, D., Mock, J. J., Justice, B. J., Cummer,
    S. A., Pendry, J. B., Starr, A. F., Smith, D. R.
    Metamaterial Electromagnetic Cloak at Microwave
    Frequencies. Science Vol. 314. no. 5801, pp. 977
    - 980 (2006).
  • Solomon, B.T. An Approach to Gravity
    Modification as a Propulsion Technology, Paper
    presented at the AIP Conference Space, Propulsion
    and Energy Sciences International Forum,
    Institute for Advanced Studies, Huntsville,
    Alabama, 24-26 February 2009.

28
Acknowledgements
  • I would like to thank the National Space Society
    for the opportunity to present this work.

29
Contact
  • Benjamin T Solomon
  • benjamin.t.solomon_at_iseti.us
  • iSETI LLC, P.O. Box 831
  • Evergreen, CO 80439
  • Call For Papers SPESIF 2010 _at_ John Hopkins
  • http//www.ias-spes.org/SPESIF.html
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