Re: Fermi "Paradox"

From: Anders Sandberg (asa@nada.kth.se)
Date: Fri Aug 01 2003 - 09:25:52 MDT

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    On Tue, Jul 22, 2003 at 06:27:14PM -0700, Robert J. Bradbury wrote:
    >
    > a) Sending a simple probe may not be sufficient -- they may be
    > allowed under "galactic club" rules -- its a self-replicating
    > probe (with directions to replicate whenever possible) that
    > may bring down lightening from the gods...

    This is actually another way of exploring the FP. The enforcement
    system has to be able to stop replicators before they get out of
    hand, and we can start constraining them by theory and maybe even
    start looking for them.

    Imagine "antibodies" spread evenly in the galaxy, detecting the
    signature of a replicator seed. They immediately launch a
    lightspeed attack on the seed; this will work only if the seed has
    not arrived at the target system, so the antibody has to be inside
    the future lightcone of the launch event and the past lightcone of
    the arrival event. Now, let the density is rho antibodies/ly^3,
    the average distance between stars are D ly and seeds travel at v.
    The spatial volume of the lightcone intersection is a somewhat
    troublesome intersection between an expanding and a contracting
    sphere (there is a formula at
    http://www.princeton.edu/~apr/articles/pre2cut/node10.html). As a
    rough approximation, the spatial volume where antibodies can act
    is ~(pi/4) D^3 (1+c/v)^2 There has to be at least one antibody per
    such volume. For the somewhat plausible v=0.3c and D=4.3 ly the
    volume is ~1000 ly^3. So the density has to be ~1e-3/ly^3 or more,
    or replicators would be able to get to other systems, disasseble
    them and launch absurd amounts of replicators elsewhere,
    overwhelming the antibodies.

    This is likely a sizeable installation, since it should be able to
    detect a small replicator seed (a nanoprobe launched with an
    interplanetary railgun?), pinpoint its trajectory and launch an
    attack that is effective over many lightyears. Sounds somewhat
    implausible, which suggests more antibodies instead. I don't know
    the effective range of lasers or similar beam weapons in
    interstellar space (something for the SDI/ABM people to think of),
    but it seems likely it is not that long compared to the distances
    between stars. Hence we should expect antibodies with an average
    distance corresponding to the effective range of their weapon
    rather than being relativistically limited - and this makes them
    much more likely to be detected. In fact, it may even be
    reasonable for the galactic club to make them relatively visible
    to interplanetary civilisations, since that way emerging civs
    might get the hint and abstain from doing something stupid.

    On the other hand, if weapons can be powerful broadsides a la
    supernovae or GRBs (like the Chenzeme of Nagata's books) then you
    only need a few of them and will likely get the civilization that
    launched them too. And it makes sense to put the antibodies in or
    near the solar systems (and brown dwarves), since that is where
    launches are likely. Hmm, my argument needs more analysis than I
    have time for...

    Anyway, considering enforcement methods over interstellar
    distances might give us a new angle to deal with the paradox.

    -- 
    -----------------------------------------------------------------------
    Anders Sandberg                                      Towards Ascension!
    asa@nada.kth.se                            http://www.nada.kth.se/~asa/
    GCS/M/S/O d++ -p+ c++++ !l u+ e++ m++ s+/+ n--- h+/* f+ g+ w++ t+ r+ !y
    


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