[ExI] Trespassing On Einstein’s Lawn

John Clark johnkclark at gmail.com
Sat Apr 23 20:56:45 UTC 2016


​I just finished ​
Amanda Gefter’s new book, Trespassing On Einstein’s Lawn,
​​
physicist Sean Carroll
​called it​
 “The most charming book ever written about the fundamental nature of
reality” and I think he’s right. Gefter is obsessed with answering the
question “why is there
​ something rather than nothing?" ; needless to say she hasn't found a
definitive answer but I have found 46 points in the book that may have some
relevance to the question:   ​

1) A good definition of "nothing" is infinite unbounded homogeneity
​.​


2)  A “thing” is defined by it’s boundaries; a blank paper is not a picture
​until
 a line is drawn
​ on it​
.

3) Godel’s Theorem is a good thing because it provides a boundary and
without a boundary there is no
​ ​
thing.

4) The boundary of a boundary is zero so everything you need to know about
the interior
​of a thing ​
is on the boundary.

5) Something and nothing are not opposites just different ways of looking
at the same thing.

6) A person’s light cone might provide the boundary to turn nothing into
something.

7) The Big Bang happened everywhere.

8) Bits are the fundamental building blocks of reality.

​9​
) Paradoxes always crop up when you try to describe physics from a God’s
eye view
​,​
so such a view can not exist.

​10​
) Spacetime curvature does not require a God’s eye view, it can be measured
from within.

11) For electromagnetism you have to expend energy to make a large
electrical charge but with gravity it’s the
​​o
pposite, it wants to make things
​
lumpy
​
so
​
unlike electromagnetism gravity
​has​
 a negative contribution to total energy in the universe.

​12​
) The universe has zero energy.

​13​
) But zero is too precise a number for
​Quantum M
echanics because
​"​
nothing
​"​
is unstable.

​14​
) The vacuum’s virtual field gives quarks 95% of their mass, the Higgs
field does the rest.

​16​
) Quantum particles don’t have positions in spacetime only probabilities.

​17​
) Something is ultimately real only if it is invariant.

​18​
) Progress in physics comes from discovering what was thought to be real is
actually observer dependent.

19) A inertial observer
​in free fall sees
a straight line through space time.

​20​
) Others see the person accelerating in a gravitational field tracing out
more and more space in less time
​. and thus​

producing​
a curved world line.

​21​
) You can turn a curve into a straight line by stretching the paper,
gravity stretches spacetime.

​22​
)
​A​
 curved world line in flat spacetime is exactly the same as a straight
world line in curved spacetime.

​23​
) A gauge force fixes the mismatch between observers, gravity is a gauge
force as are all the fundamental forces in physics.

​24​
) The local curvature of spacetime cancels out energy and momentum
​,​
and that’s why mass curves spacetime.

​25​
) In General
​R​
elativity
​m​
ass (and
​because E=MC^2​
 energy
​ too​
) is only defined within reference frames, it is observer dependent.

​26​
) Entropy is a measure of hidden information
​,​
and a event horizon can hide information.

​27​
) Entropy is not conserved.

​28​
) The more symmetric something is the less information it contains.

​29​
) The Entropy of nothing is zero.

​30​
) The very early universe was smooth and
​symmetrical​
 and thus had low Entropy.

​31​
) Gravity wants to make the universe lumpy and thus increase it’s Entropy.

​32​
) The maximum number of bits of information inside a sphere is equal to one
fourth the area of the surface in Planck Areas.

​33​
)
​A​
 Black Hole
​contains as much information as any volume can, ​although its
 amount is proportional to
​the Black Hole's​
 surface not its volume.

​34​
)
​ ​
Hawking radiation is observer dependent.

​35)​
 A unmeasured bit of quantum information can not be perfectly copied, if
you could then you could outsmart the uncertainty principle.

​36​
) Quantum Mechanics says information can’t be destroyed but
​General Relativity says it can be, the confrontation comes to a head in ​
Black Holes.

​37​
) A outside observer would say information never crosses the Event Horizon
​of a Black hole ​
but stays on the surface.

​38​
) A observer falling into the Black Hole would say information
​does ​
cross the Event Horizon without incident and nothing unusual happens until
the Singularity
​ is reached​
.

​39​
) A black hole the mass of our sun,  would take about 10^67 years to
evaporate by Hawking Radiation.

​40​
) Hawking Radiation contains information on what went into a Black Hole.

​41​
) The time needed to decode Hawking Radiation increases exponentially even
with a Quantum Computer.

​42​
) It would take not 10^67 but 10^10^67 years to compute what went into the
Black Hole from the Hawking Radiation that came out of it, and the Black
Hole would be long gone by then.

​43​
) The location of information is observer dependent, so nobody can see the
same quantum bit at 2 different locations at the same time because
​n​
o observer can see both inside and outside a Black Hole horizon at the same
time.

4
​4​
) If Quantum Mechanics and General Relativity don’t contradict each other
​
that must mean that if you haven’t
​finished the computation
then
​the information is​
 not there yet.

​45)​
The only thing that's invariant is nothing

​46) ​
Reality is observer dependent, and the weirdness in physics doesn’t come
from non-locality but
​from ​
non-reality.

​ John K Clark​
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