SETI public: The End of the Universe Will Not Be Pleasant

From: LARRY KLAES (ljk4_at_msn.com)
Date: Fri Mar 07 2003 - 09:13:33 PST

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    THE END MIGHT BE NIGH IN 20 BILLION YEARS

    >From Space.com, 6 March 2003

    http://www.space.com/scienceastronomy/big_rip_030306.html

    The Big Rip: New Theory Ends Universe by Shredding Everything

    By Robert Roy Britt

    A rather harrowing new theory about the death of the universe paints a
    picture of "phantom energy" ripping apart galaxies, stars, planets and
    eventually every speck of matter in a fantastical end to time.

    Scientifically it is just about the most repulsive notion ever conceived.

    The speculative but serious cosmology is described as a "pretty fantastic
    possibility" even by its lead author, Robert Caldwell of Dartmouth
    University. It explains one possible outcome for solid astronomical
    observations made in the late 1990s -- that the universe is expanding at an
    ever-increasing pace, and that something unknown is vacuuming everything
    outward.

    The question Caldwell and his colleagues posed is, what would happen if the
    rate of acceleration increased?

    Their answer is that the eventual, phenomenal pace would overwhelm the
    normal, trusted effects of gravity right down to the local level. Even the
    nuclear forces that bind things in the subatomic world will cease to be
    effective.

    "The expansion becomes so fast that it literally rips apart all bound
    objects," Caldwell explained in a telephone interview. "It rips apart
    clusters of galaxies. It rips apart stars. It rips apart planets and solar
    systems. And it eventually rips apart all matter."

    He calls it, as you might guess, the Big Rip.

    The standard view

    Driving the known acceleration of the universe's expansion is a mysterious
    thing is called dark energy, thought of by scientists as anti-gravity
    working over large distances.

    Conventional wisdom holds that the acceleration will proceed at a constant
    rate, akin to a car that moves 10 mph faster with each mile traveled. With
    nothing to cap the acceleration, all galaxies will eventually recede from
    one another at the speed of light, leaving each galaxy alone in a cold, dark
    universe within 100 billion years. We would not be able to see any galaxies
    outside our Milky Way, even with the most powerful telescopes.

    That's the conventional view, remarkable as it sounds.

    The Big Rip theory has dark energy's prowess increasing with time, until
    it's an out-of-control phantom energy. Think of our car accelerating an
    additional 10 mph every half mile, then every hundred yards, then every
    foot.

    Before long, the bumpers are bound to fly off. Sooner or later, our
    hypothetical engine will come apart, regardless of how much we spend on
    motor oil.

    Countdown to demise

    Other theorists who have reviewed the Big Rip theory are not yet sold on the
    idea. Meanwhile, Caldwell's team has provided a precise countdown to total
    demise. The projected end is, reassuringly, 20 billion years away. If our
    species survives the next 19 billion years (and there are serious doubts
    about this, given our Sun's projected fate) here are some signs that
    scientists of the future will want to look for.

    A billion years before the end, all galaxies will have receded so far and so
    fast from our own as to be erased from the sky, as in no longer visible.

    When the Milky Way begins to fly apart, there are 60 million years left.

    Planets in our solar system will start to wing away from the Sun three
    months before the end of time.

    When Earth explodes, the end is momentarily near.

    At this point, there is still a short interval before atoms and even their
    nuclei break apart. "There's about 30 minutes left," Caldwell said, "But
    it's not quality time."

    And then what? Does the universe recycle itself? Is there something after
    nothing?

    "We're not sure what happens after that," Caldwell says. "On the face of it,
    it would look like time ends."

    The first explosion

    Caldwell's study had humble beginnings. He and his colleagues, Marc
    Kamionkowski and Nevin Weinberg at Caltech, were considering how a sphere of
    matter collapses under its own weight to form a galaxy. In computer models,
    they tweaked with the dark energy factor and found that too much of it would
    actually prevent the sphere from collapsing. In extreme cases, the sphere
    exploded.

    "That was our hint that there was something really unusual going on,"
    Caldwell said.

    It wasn't long ago, just before the accelerated expansion was discovered,
    that many cosmologists believed the universe might reverse course, that
    normal gravity would win, and that everything would fall back in a Big
    Crunch. More recently, solid observational data has all but assured the
    infinite-expansion model and the cold, dark, never-ending end.

    The Caldwell group decided there might be a third possibility, leading to
    their new paper, which has been submitted to the Physical Review.

    But there are many unknowns. It is not clear if the dark energy driving
    expansion is a force not currently described by physics, or if it is merely
    a different manifestation of gravity over huge distances. The repulsion
    could be a response to dark matter, unseen stuff that is known to comprise
    23 percent of the universe, based on firm observations.

    Dark matter has unknown properties, and it may be related to dark energy,
    Caldwell said. He notes that even Einstein considered that gravity might
    work repulsively, in a manner consistent with his theory of general
    relativity.

    Dark energy, being quantified only recently, tends to be discussed as some
    strange new force, in addition to the four fundamental forces: gravity,
    electromagnetism, and the strong and weak nuclear forces that govern atoms.
    But the repulsion is possibly just the way gravity behaves in the presence
    of dark energy, Caldwell said. In that sense, it is not a new force.

    Cautious reception

    To turn dark energy into destructive phantom energy, Caldwell and his
    colleagues had to play around with a thing called the cosmological constant,
    a mathematical fix that Einstein applied to general relativity. Einstein
    later called it his greatest mistake, when Edwin Hubble found in the 1920s
    that the universe was expanding (seven decades later, that expansion would
    be seen accelerating).

    The cosmological constant has been recently revived. Attempts to describe
    dark energy differ in how the density of dark energy varies with time. In
    some models, the density decreases slowly. For the cosmological constant,
    the density is a constant. For phantom energy, it must grow with time.

    "We considered a more exotic form of dark energy which was more repulsive,"
    as Caldwell explains is.

    Abraham Loeb, a theoretician at the Harvard-Smithsonian Center for
    Astrophysics, has quantified the lonely effects of a forever-expanding
    universe. Loeb stands by that scenario, but he said Caldwell's idea is
    nonetheless interesting to explore.

    "I think it's a logical possibility," Loeb told SPACE.com. But he cautioned
    that altering the cosmological constant goes against current consensus.

    "If I had to place a bet, I would bet in favor of the standard cosmological
    constant," Loeb said.

    Sci-fi to reality

    If Caldwell's team is right, cosmology would undergo a revolution. Sci-fi
    ideas like wormholes and time travel might suddenly enter the realm of hard
    science. All of this could sort itself out pretty soon, Caldwell believes.
    Observations over the next few years may actually show whether his phantom
    energy is possible.

    "Who knows if it is right or wrong," Caldwell said of his theory. "I think
    we'll find out pretty soon."

    In fact, recent observations from NASA's WMAP space probe have pinned down
    the physics of the universe with surprising accuracy. A little wiggle room
    remains for the cosmological constant. Yet more WMAP data are expected over
    the next four years. Other missions, including one called the Supernova
    Acceleration Probe (SNAP), could provide answers, Caldwell said.

    Even if the Big Rip is a big bust, there's no guarantee of a pleasant
    ending.

    Alternate final chapter

    Paul Steinhardt, a Princeton University physicist, is, like Caldwell and
    Loeb, no stranger to strange ideas. Steinhardt advocates a cyclical
    universe, one that has no beginning or end but which instead is constantly
    starting over again.

    Steinhardt theorizes within the generally accepted standards of the
    cosmological constant. He said the Big Rip is more exotic than most ideas
    but still conceivable, a projected possible result that is "straightforward
    and obvious for cosmologists."

    Yet there is another entirely different possibility for the final moments of
    time as we know it.

    In a theory put forth two years ago by Steinhardt and his colleagues, our
    universe is but a membrane, or brane, floating in a five-dimensional space.
    It is destined to collide dramatically with another brane. The idea, labeled
    the Ekpyrotic Universe, would replace portions of the Big Bang scenario
    while sticking to the presently accepted estimates of acceleration.

    "Lest you get too optimistic, galaxies are destroyed in a far more violent
    way," Steinhardt said of the brane scenario. "They are vaporized at the next
    'bang' -- the collision between branes ... so, you either rip them apart or
    you vaporize them."


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