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) in classical gravitational fields. Indeed it is more natural to express the effect in terms of the quantity g, the gravitational acceleration near Earth's surface, which is the relevant aspect of the experimental environment, and then 0, which indicates intrinsically gravitational dynamics, does not
with a scalar field in an almost flat potential. If one considers a quantized approximately massless scalar field in de-Sitter space, expanded into Fourier components with quantized mode functions, vk then it is straightforward to calculate the zero-point quantum fluctuations of these mode functions, (
culation by some theoretical cosmologists that the universe comes in an infinite number of copies which contain many exact and inexact copies of the Earth and each one of usil 1 Within the present proposal. the fact that macroscopic bodies do not appear to satisfy the superposition principle can be tak
4-4‘1))ba) = Loa + Z ( n°) ti(e",-.6)),„b nb where ok, = Va. and Rafr and 'lid, satisfy the properties above. We can now expand & I, and thd, in Fourier series. (23) (24) R.(e1(‘ -ta)ab = RI, s111`.(n(4ki + 0:1,b) (25) ?MG EFTA_R1_02022336 EFTA02688810 8 CO u (eOrt)),,b = I Cbcos0(4). — (
rtainty principle, as the energy it can carry is so small that no visible violation of the conservation of en- ergy will occur. Thus, an electron on Earth can emit a virtual photon that could travel to Alpha Centauri, four light-years away, and that pho- ton can still produce a force on an electron the
ics of sounds." Fermi submitted an "essay" that included solving partial differential equations for a vibrating rod and applying a technique called Fourier analysis. Even today, these mathematical techniques are not normally encountered until maybe the third year of an undergraduate degree, and for som
Entities connected to both Earth and Fourier

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Harvey Weinstein
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Bradley Cooper
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Eric Schmidt
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Bradley Edwards
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Freeman Dyson
PERSONQuantum
ORGANIZATION
Martin Nowak
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Bristol
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PERSONLos Alamos
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Joscha Bach
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