SETI public: Universe as Doughnut: New Data, New Debate

From: LARRY KLAES (ljk4_at_msn.com)
Date: Sun Mar 16 2003 - 18:03:54 PST

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    Universe as Doughnut: New Data, New Debate

    March 11, 2003
    By DENNIS OVERBYE

    Long ago in the dawn of the computer age, college students
    often whiled away the nights playing a computer game called
    Spacewar. It consisted of two rocket ships attempting to
    blast each other out of the sky with torpedoes while trying
    to avoid falling into a star at the center of the screen.

    Although cartoonish in appearance, the game was amazingly
    faithful to the laws of physics, complete with a
    gravitational field that affected both the torpedoes and
    the rockets. Only one feature seemed outlandish: a ship
    that drifted off the edge of the screen would reappear on
    the opposite side.

    Real space couldn't work that way.

    Or could it?

    Imagine that the Spacewar screen is wrapped
    around to form a cylinder or a section of a doughnut so
    that the two edges meet.

    That is the picture of space, some cosmologists say, that
    has been suggested by a new detailed map of the early
    universe. Their analysis of this map has now provided a
    series of hints - though only hints - that the universe may
    have a more complicated shape than astronomers presumed.

    Rather than being infinite in all directions, as the most
    fashionable theory suggests, the universe could be
    radically smaller in one direction than the others. As a
    result it may be even be shaped like a doughnut.

    "There's a hint in the data that if you traveled far and
    fast in the direction of the constellation Virgo, you'd
    return to Earth from the opposite direction," said Dr. Max
    Tegmark, a cosmologist at the University of Pennsylvania.

    The new data have generated both buzz and skepticism among
    cosmologists in recent weeks. Dr. Tegmark and other
    astronomers agree that the measurements are far from
    conclusive, or even persuasive about the shape of the
    universe.

    But if true, the doughnut universe would force cosmologists
    to reconsider their theories about what happened in the
    earliest moments after the universe was born in the Big
    Bang; those theories predict an infinite cosmos.

    The new findings have brought to center stage the hope that
    astronomers may be able to test speculations about the
    shape, or topology, of the universe that until recently
    have been relegated to the abstract mathematical margins of
    cosmology.

    The results are part of the bounty of data produced by a
    NASA satellite known as the Wilkinson Microwave Anisotropy
    Probe, built and operated by an international collaboration
    led by Dr. Charles L. Bennett of the Goddard Space Flight
    Center in Greenbelt, Md. The satellite recorded the pattern
    of heat, in the form of faint microwave radiation, that
    fills the sky.

    This radiation is believed to be the afterglow of the Big
    Bang itself, and thus constitutes a portrait of the
    universe when it was only 380,000 years old.

    As the COBE satellite first confirmed in 1992, the
    microwave cloud is laced with ripples and splotches - lumps
    in the cosmic gravy - from which galaxies and other cosmic
    structures would ultimately form.

    According to theory, these lumps are born as microscopic
    fluctuations during the first instant of time and then
    amplified into sound waves as the universe expands and
    matter and energy slosh around.

    Now the new satellite has illuminated the findings of COBE
    (pronounced KOE-bee, for Cosmic Background Explorer) in
    exquisite detail.

    By analyzing these waves cosmologists can determine many of
    the characteristics of the universe, which scientists have
    long debated, like its age and density. To their delight,
    the first results from the Wilkinson satellite, released
    last month, confirmed many of the strange ideas that
    cosmologists entertained in the last decade, including the
    notion that most of the universe consists of something
    called dark energy, which is pushing space apart at an
    accelerating rate.

    "Cosmologists have built a house of cards and it stands,"
    said Dr. James Peebles, a cosmologist at Princeton.

    But to their even greater delight, perhaps, as they dig
    into the trove released last month, cosmologists are
    finding hints of even more strangeness.

    In principle, in an infinite universe, the waves in the
    cosmic fireball should appear randomly around the sky at
    all sizes. But, according to the new map, there seems to be
    a limit to the size of the waves, with none extending more
    than 60 degrees across the sky.

    The effect was first noted as a puzzle in the COBE data,
    according to Dr. Gary Hinshaw, an astronomer at the Goddard
    Space Flight Center and a member of the Wilkinson probe
    team, and now seems confirmed.

    If the universe were a guitar string, it would be missing
    its deepest notes, the ones with the longest wavelengths,
    perhaps because it is not big enough to sustain them.

    "The fact that there appears to be an angular cutoff hints
    at a special distance scale in the universe," Dr. Hinshaw
    said.

    Another analysis of the new map suggests that there is a
    special direction, as well as a special scale in the
    universe. While reanalyzing the Wilkinson data to eliminate
    radio noise from stars and our own galaxy, Dr. Tegmark, Dr.
    Angélica de Oliveira-Costa, also at Pennsylvania and
    married to Dr. Tegmark, and Dr. Andrew J. S. Hamilton of
    the University of Colorado have discovered that the
    universe appears lumpier in one direction through space
    than it does in another. When they combed finer variations
    out of the map, the remaining large-scale variations formed
    a line across the sky.

    It could be a chance alignment, a statistical fluke, Dr.
    Tegmark said, or contamination from radio noise from the
    galaxy.

    But in a paper posted on the physics Web site (at
    arXiv.org/pdf /astro-ph/0302496) late last month, the three
    cosmologists wrote that it was "difficult not to be
    intrigued" that their results bore all the earmarks of what
    are variously called small, compact, finite or periodic
    universes.

    If the universe is finite in one dimension, like a cylinder
    or a doughnut, Dr. Tegmark said in an interview, there is a
    limit to the size of clumps that can fit in that direction.
    They couldn't be bigger than the universe in that
    direction, just as a guitar string can only play a note so
    low, depending on its length. So the biggest blobs would
    have to squish out in a plane in other directions. The way
    home around the doughnut would be perpendicular to that
    plane.

    Nobody is yet claiming that this is a revolution. The
    notion of a special direction is on less firm ground than
    the discovery of a cutoff of large structures. "More
    detailed work in needed to clarify what's going on," Dr.
    Tegmark said.

    Dr. Martin Rees, a cosmologist at Cambridge University,"
    said he didn't think there was evidence for "anything
    crazy" in the data.

    Even aficionados of finite universes are guarded. Dr. David
    Spergel, a Princeton cosmologist and Wilkinson satellite
    team member, called the results "intriguing," but cautioned
    that they could also be due to chance.

    Dr. Hinshaw called the findings of Dr. Tegmark's team
    "surprisingly robust," but added, "I'm not sure it says
    something profound about the universe."

    Dr. Alexei Starobinski, a theorist at the Landau Institute
    in Moscow, proposed in 1984 with his mentor, Dr. Yakov B.
    Zeldovich, that the universe could have been born as a
    doughnut. Dr. Starobinski emphasized that an infinite
    universe with ordinary Euclidean geometry was the most
    natural universe and still favored by theory.

    "However, theory is theory, but observations might tell us
    something different," he said in an e-mail message.

    The Science of Shapes
    A Compact Universe
    Like Mirrored
    Halls

    The new work involves topology, the branch of mathematics
    that deals with shapes. Topologists are often accused of
    not knowing the difference between a coffee mug and a
    doughnut; because each object has one hole, the two can be
    deformed into each other and are thus topologically
    equivalent. In a similar vein, a figure 8 and a pair of
    eyeglass frames are also the same to a topologist. The more
    holes, the more complicated the topology.

    The simplest topology is just the infinite space of the
    Euclidean geometry taught in high school. But some
    cosmologists have a hard time calculating how an infinite
    universe could have appeared in that kind of space. Nature,
    they contend, might have had an easier time making a small
    "compact" universe than an infinite one, and they assume
    Nature would take the easy way out.

    "The basic idea is that God's on a budget," said Dr. George
    Smoot, a physicist at the University of California's
    Lawrence Berkeley Laboratory and a leader on the COBE team.

    The simplest of these compact universes is something called
    a 3-torus, a doughnut wrapped in three different
    dimensions. This object is essentially impossible to
    visualize: it is the equivalent, in a way, of a cube whose
    opposite sides are somehow glued together. In two
    dimensions it works just like the Spacewar screen.

    Living in such a universe would be like being inside a hall
    of mirrors, Dr. Tegmark said. Instead of seeing new stars
    deeper and deeper in space, you see the same things over
    and over again as light travels out one side of your cube
    and back in the other.

    This mirror game is not limited to cubes and doughnuts.
    Over the years mathematicians, particularly Dr. William
    Paul Thurston, now at the University of California at
    Davis, and Dr. Jeffrey Weeks, an independent mathematician,
    have speculated about universes composed of various
    polyhedrons glued together in various ways.

    In 1996 the French astronomer Dr. Jean-Pierre Luminet of
    the Paris Observatory and his colleagues Dr. Roland Lehoucq
    and Dr. Marc Lachieze-Rey, both of the Center for
    Astrophysical Studies in Saclay, France, developed a method
    called "cosmic crystallography," using galaxy statistics to
    detect and diagnose the repeating periodic patterns that
    would be created in the sky by light going around and
    around in differently shaped universe.

    Finite or Infinite?
    Problems Are Posed
    For Favored Theory

    Why would the universe want to do this to us? Partly to
    avoid the difficulties of the infinite, said Dr. Glenn
    Starkman, an astronomer at the Case Western Reserve
    University in Cleveland. Besides being difficult to create,
    an infinite universe is philosophically unattractive. In an
    infinite volume, he pointed out, anything that can happen
    will happen.

    "Somewhere there are two guys having this same
    conversation," Dr. Starkman said in a telephone interview,
    "except that one of them has a purple phone."

    Moreover, the idea that dimensions could be curled in loops
    occurs naturally in theories that try to unite gravity and
    particle physics, several physicists pointed out. For
    example, according to string theory, the leading candidate
    for a theory of everything, the universe actually has 10
    dimensions - 9 of space and 1 of time - rather than the 4
    we are familiar with. The extra dimensions are curled up
    into submicroscopic loops, like the threads in an uncut
    carpet pile, so that we don't notice them in ordinary life.

    "This is the same idea on a very large scale," Dr. Smoot
    said.

    Knowing that all nine of the spatial dimensions predicted
    by string theory are finite and thus on the same footing
    could help string theorists decide among the nearly endless
    possibilities allowed by the theory, scientists say.

    But a finite universe would create big problems for the
    reigning theory of the Big Bang, inflation theory. It
    posits that the universe underwent a burst of
    hyperexpansion in its earliest moments. Among other things,
    it implies that the observable universe today, a bubble 28
    billion light-years in diameter, is only a speck on the
    surface of a vastly greater realm trillions upon trillions
    of light-years across.

    "There's no natural way yet proposed to get the inflation
    to stop and give a space that's big enough to house all the
    galaxies but small enough to see within the observable
    horizon," said Dr. Janna Levin, a Cambridge University
    cosmologist who wrote about finite universes in her 1992
    book, "How the Universe Got Its Spots, Diary of a Finite
    Time in a Finite Space."

    Dr. Spergel added, "If the universe were finite, then this
    would rule out inflation and require something new."

    The Search for Patterns
    One Convincing Sign
    Of the
    Doughnut

    So far, sporadic searches for repeating patterns of quasars
    or distant galaxy clusters that would occur in a hall of
    mirrors universe have been unsuccessful.

    For finite universe aficionados, the first encouragement of
    note was COBE's discovery that the universe appeared to be
    deficient in large-scale fluctuations. There were no
    structures extending more than about 60 degrees across the
    sky. But the finding was subject to large statistical
    uncertainties, astronomers said.

    There are other possible explanations for the cutoff in
    fluctuation size, Dr. Starkman explained. According to
    inflation the biggest longest waves are created first, and
    thus the missing notes are the earliest ones that would
    have been strummed by inflation's guitar. Perhaps, he said,
    this is telling us something about the beginning of
    inflation.

    Dr. George Efstathiou of Cambridge University has pointed
    out in a recent paper submitted to the Monthly Notices of
    the Royal Astronomical Society that the Wilkinson satellite
    data are also marginally consistent with yet another finite
    shape, namely a sphere. In that case, fluctuations larger
    than the radius of the sphere might be dampened, he said,
    producing the observed cutoff.

    The most convincing sign of a doughnut universe, if it
    exists, astronomers say, could come from a search of the
    satellite data now being performed by Dr. Spergel, Dr.
    Starkman and Dr. Neil J. Cornish of Montana State
    University. "We're looking for circles in the sky," Dr.
    Starkman said.

    In a 1998 paper they point out that if the universe is
    small enough, part of the cosmic background radiation,
    which essentially fills the sky surrounding us, will hit
    the sides of the "box" or the space war screen we are in
    and appear on the other side. The result, in the simplest
    case, would be identical circles on opposite sides of the
    sky with the same patterns of hot and cold running around
    them.

    In the simplest case, the size of the circles would depend
    on the distance between the "walls" of the universe: the
    smaller the universe, the bigger the circles.

    Success or even a definitive failure is not guaranteed. "It
    would be fantastic if something like that was found," Dr.
    Hinshaw said of the circles.

    But success or even a definitive failure is not guaranteed.
    If the universe is finite but still much larger than
    today's observable universe - 28 billion light-years in
    diameter - the circles will not show. "Usually in science
    when we see an intriguing pattern that appears to
    contradict existing theory we do a better experiment," Dr.
    Spergel wrote in an e-mail message, but in this case,
    "Ultimately we will be limited by the fact that we can only
    observe the `visible' universe."

    Dr. Levin was doubtful, "I suspect every last one of us
    would be flabbergasted if the universe was so small," she
    said in an e-mail message. When she first heard about the
    new satellite data, she reported, "I tried on the idea that
    we were really and truly seeing the finite extent of space
    and I was filled with dread.

    "But I'm enjoying it too."

    http://www.nytimes.com/2003/03/11/science/space/11COSM.html?ex=1048865986&ei=1&en=027a4a37d961f1fc


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