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Polarizable vacuum

Polarizable vacuum is a physics topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Polarizable vacuum rather than just read about it. In short: In theoretical physics, particularly fringe physics, polarizable vacuum (PV) and its associated theory refer to proposals by Harold Puthoff, Robert H. Dicke, and others to develop an analog of general relativity to describe gravity and its relationship to electromagnetism.

Key takeaways

  • Polarizable vacuum belongs to physics; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Polarizable vacuum to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Polarizable vacuum from memory before moving on to harder problems.

Reference excerpt

In theoretical physics, particularly fringe physics, polarizable vacuum (PV) and its associated theory refer to proposals by Harold Puthoff, Robert H. Dicke, and others to develop an analog of general relativity to describe gravity and its relationship to electromagnetism.

Description In essence, Dicke and Puthoff proposed that the presence of mass alters the electric permittivity and the magnetic permeability of flat spacetime, εo and μo respectively by multiplying them by a scalar function, K:

ε 0 → ε = K ε 0 ; μ 0 → μ = K μ 0 {\displaystyle \varepsilon _{0}\to \varepsilon =K\varepsilon _{0}\;;\;\mu _{0}\to \mu =K\mu _{0}}

arguing that this will affect the lengths of rulers made of ordinary matter so that in the presence of a gravitational field, the spacetime metric of Minkowski spacetime is replaced by

d s 2 = − 1 κ 2 d t 2 + κ 2 ( d x 2 + d y 2 + d z 2 ) {\displaystyle ds^{2}=-{\frac {1}{\kappa ^{2}}}dt^{2}+\kappa ^{2}\,(dx^{2}+dy^{2}+dz^{2})}

where κ 2 = K {\displaystyle \kappa ^{2}=K} is the so-called "dielectric constant of the vacuum". This is a "diagonal" metric given in terms of a Cartesian chart and having the same stratified conformally flat form in the Watt-Misner theory of gravitation. However, according to Dicke and Puthoff, κ must satisfy a field equation that differs from the field equation of the Watt-Misner theory. In the case of a static spherically symmetric vacuum, this yields the asymptotically flat solution

κ = exp ⁡ ( m / r ) = 1 + m / r + O ( 1 r 2 ) {\displaystyle \kappa =\exp(m/r)=1+m/r+O\left({\frac {1}{r^{2}}}\right)}

The resulting Lorentzian spacetime agrees with the analogous solution in the Watt-Misner theory. It has the same weak-field limit and far-field as the Schwarzschild vacuum solution in general relativity. It satisfies three of the four classical tests of relativistic gravitation (redshift, deflection of light, precession of the perihelion of Mercury) to within the limit of observational accuracy. However, as shown by Ibison (2003), it yields a different prediction for the inspiral of test particles due to gravitational radiation. However, requiring stratified-conformally flat metrics rules out the possibility of recovering the weak-field Kerr metric and is certainly inconsistent with the claim that PV can give a general "approximation" of the general theory of relativity. In particular, this theory exhibits no frame-dragging effects. Also, the impact of gravitational radiation on test particles differs profoundly between scalar theories and tensor theories of gravitation, such as general relativity. LIGO is not intended primarily as a test ruling out scalar theories. However, it is widely expected to do so as a side benefit once it detects unambiguous gravitational wave signals exhibiting the characteristics expected in general relativity. Ibison has considered a "cosmological solution" of PV, analogous to the Friedmann dust solution with flat orthogonal hyperslices in general relativity, and argues that this model is inconsistent with various observational and theoretical constraints. He also finds a rate of inspiral disagreeing with observation. The latter result disagrees with that of Watt and Misner, whose Lorentzian manifold differs from PV in the case of cosmology. Contrary to Puthoff's claims, it is widely accepted that no scalar theory of gravitation can reproduce all of general relativity's successes. It might be noted that De Felice uses constitutive relations to obtain a susceptibility tensor which lives in spatial hyperslices; this provides extra degrees of freedom, which help make up for the degree of freedom lacking in PV and other scalar theories.

Criticism Puthoff himself has offered various characterizations of his proposal, which has been variously characterized as

an attempt to reformulate general relativity in terms of a purely formal analogy with the propagation of light through an optical medium, an attempt to replace general relativity with a scalar theory of gravitation featuring formal analogies with Maxwell's theory of electromagnetism, an attempt to unify gravitation and electromagnetism in a theory of electrogravity, an attempt to provide a physical mechanism for how spacetime gets curved in general relativity, which suggests (to Puthoff) the possibility of "metric engineering" for such purposes as spacecraft propulsion (see Breakthrough Propulsion Physics Program). PV has origins in more mainstream work by such physicists as Robert Dicke. Still, in current parlance, the term does appear to be most closely associated with the speculations of Puthoff. The claims have not been accepted in mainstream physics. Mainstream physicists agree that PV is

not viable as a unification of gravitation and electromagnetism not a "reformulation" of general relativity, not a viable theory of gravitation since it violates observational and theoretical requirements.

… excerpt ends here. Continue reading the full article.

Worked examples

Example 1 — a first encounter with Polarizable vacuum

Start with the simplest possible case. Write down what Polarizable vacuum claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In physics, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Polarizable vacuum before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Polarizable vacuum ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Polarizable vacuum

In research
Polarizable vacuum appears in physics research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Polarizable vacuum in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Polarizable vacuum is common in secondary-school and first-year university syllabi. It links to neighbouring topics Fringe physics, Theories of gravity, so understanding it makes those chapters shorter.
In everyday life
Look for Polarizable vacuum outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Polarizable vacuum in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Polarizable vacuum means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Polarizable vacuum out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Polarizable vacuum in simple terms?

In theoretical physics, particularly fringe physics, polarizable vacuum (PV) and its associated theory refer to proposals by Harold Puthoff, Robert H. Dicke, and others to develop an analog of general relativity to describe gravity and its relationship to electromagnetism.

Why does Polarizable vacuum matter?

Because it connects several physics ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Polarizable vacuum?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Polarizable vacuum.

Tags

  • Fringe physics
  • Theories of gravity

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