SETI bioastro: FW: NYTimes.com Article: From Space, a New View of Doomsday

From: LARRY KLAES (ljk4_at_msn.com)
Date: Tue Feb 17 2004 - 06:54:59 PST

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    >From Space, a New View of Doomsday
    >
    >February 17, 2004
    > By DENNIS OVERBYE
    >
    >
    >
    >
    >
    >Once upon a time, if you wanted to talk about the end of
    >the universe you had a choice, as Robert Frost put it,
    >between fire and ice.
    >
    >Either the universe would collapse under its own weight one
    >day, in a fiery "big crunch," or the galaxies, now flying
    >outward from each other, would go on coasting outward
    >forever, forever slowing, but never stopping while the
    >cosmos grew darker and darker, colder and colder, as the
    >stars gradually burned out like tired bulbs.
    >
    >Now there is the Big Rip.
    >
    >Recent astronomical
    >measurements, scientists say, cannot rule out the
    >possibility that in a few billion years a mysterious force
    >permeating space-time will be strong enough to blow
    >everything apart, shred rocks, animals, molecules and
    >finally even atoms in a last seemingly mad instant of
    >cosmic self-abnegation.
    >
    >"In some ways it sounds more like science fiction than
    >fact," said Dr. Robert Caldwell, a Dartmouth physicist who
    >described this apocalyptic possibility in a paper with Dr.
    >Marc Kamionkowski and Dr. Nevin Weinberg, from the
    >California Institute of Technology, last year.
    >
    >The Big Rip is only one of a constellation of doomsday
    >possibilities resulting from the discovery by two teams of
    >astronomers six years ago that a mysterious force called
    >dark energy seems to be wrenching the universe apart.
    >
    >Instead of slowing down from cosmic gravity, as
    >cosmologists had presumed for a century, the galaxies
    >started speeding up about five billion years ago, like a
    >driver hitting the gas pedal after passing a tollbooth.
    >
    >Dark energy sounded crazy at the time, but in the
    >intervening years a cascade of observations have
    >strengthened the case that something truly weird is going
    >on in the sky. It has a name, but that belies the fact that
    >nobody really knows what dark energy is.
    >
    >In six years it has become one of the central and
    >apparently unavoidable features of the cosmos, the surprise
    >question mark at the top of everybody's list, undermining
    >what physicists presumed they understood about space, time,
    >gravity and the future of the universe.
    >
    >"In five years we've gone from saying it looks like a
    >mistake to something that everyone is claiming evidence
    >for," said Dr. Robert Kirshner of the Harvard-Smithsonian
    >Center for Astrophysics, who was part of the original
    >discovery.
    >
    >Dr. Saul Perlmutter, a physicist from the Lawrence Berkeley
    >Laboratory who was a leader of one of the 1998 teams, said
    >he thought astronomers had even gotten comfortable with the
    >idea - "or as comfortable as you can be with something as
    >bizarre as dark energy."
    >
    >Now, armies of astronomers are fanning out into the night,
    >enlisting telescopes, large and small, from Chile to Hawaii
    >to Arizona to outer space, in a quest to take the measure
    >of dark energy by tracing the history of the universe with
    >unprecedented precision.
    >
    >Some of them are following the trail blazed by the first
    >two groups six years ago, searching out a kind of exploding
    >star known as Type 1a the supernova. Those stars serve as
    >markers in space, enabling scientists to plumb the size of
    >the universe and how it grew over time. Where the first
    >groups based their conclusions on observing a few dozen
    >supernovas, the new efforts intend to harvest hundreds or
    >thousands of them.
    >
    >Others are seeking to gain leverage by investigating how
    >the antigravitational force of dark energy has retarded the
    >growth of conglomerations of matter like galaxies. In one
    >ambitious project, a team led by Dr. John Carlstrom of the
    >University of Chicago is building an array of radio
    >telescopes at the South Pole to count and study clusters of
    >galaxies deep in space-time. Others are already probing the
    >internal dynamics of galaxies by the thousands, or building
    >giant cameras that use the light-bending powers of gravity
    >itself as lenses to map invisible dark matter in space and
    >compile a growth chart of cosmic structures.
    >
    >Dr. Anthony Tyson, now at Bell Laboratories, is head of a
    >project to build a "dark matter telescope" known as the
    >Large Synoptic Survey Telescope. "High energy physicists
    >have been marching into our project," he said. "This is not
    >just another telescope. It's a physics experiment, like a
    >particle accelerator."
    >
    >After all, the fate of the universe is at stake. If the
    >dark energy is virulent enough, then that fate "is quite
    >fantastic and completely different than the possibilities
    >previously discussed," Dr. Caldwell and his colleagues
    >wrote last year.
    >
    >The Search for One Number
    >
    >The idea of an antigravitational force pervading the cosmos
    >does sound like science fiction, but theorists have long
    >known that certain energy fields would exert negative
    >pressure that would in turn, according to Einstein's
    >equations, produce negative gravity. Indeed, some kind of
    >brief and violent antigravitational boost, called
    >inflation, is thought by theorists to have fueled the Big
    >Bang.
    >
    >As they try to figure out how this strange behavior could
    >be happening to the universe today, astronomers say the
    >ultimate prize from all the new observing projects could be
    >as simple as a single number.
    >
    >That number, known as w, is the ratio between the pressure
    >and density of dark energy. Knowing this number and how it
    >changes with time - if it does - might help scientists pick
    >through different explanations of dark energy and thus the
    >future of the universe - "whether it's gonna lead to a Big
    >Rip, a Big Collapse or just a Big Fizzle," as Dr. Adam
    >Riess of the Space Telescope Science Institute in Baltimore
    >put it in an e-mail message.
    >
    >One possible explanation for dark energy, perhaps the
    >sentimental favorite among astronomers, is a force known as
    >the cosmological constant, caused by the energy residing in
    >empty space. It was first postulated back by Einstein in
    >1917. A universe under its influence would accelerate
    >forever.
    >
    >While the density of energy in space would remain the same
    >over the eons, as the universe grows there would be more
    >space and thus more repulsion. Within a few billion years,
    >most galaxies would be moving away from our own faster than
    >the speed of light and so would disappear from the sky; the
    >edge of the observable universe would shrink around our
    >descendants like a black hole.
    >
    >But attempts to calculate the cosmological constant using
    >the most high-powered modern theories of gravity and
    >particle physics result in numbers 1060 times as great as
    >the dark energy astronomers have observed - big enough, in
    >fact, to have blown the universe apart in the first second,
    >long before even atoms had time for form. Theorists admit
    >they are at a loss. Perhaps, some of them now say,
    >Einstein's theory of gravity, the general theory of
    >relativity, needs to be modified.
    >
    >Another possibility comes from string theory, the putative
    >theory of everything, which allows that space could be
    >laced with other energy fields, associated with particles
    >or forces as yet undiscovered. Those fields, collectively
    >called quintessence, could have an antigravity effect.
    >Quintessence could change with time - for example, getting
    >weaker and eventually disappearing as the universe expanded
    >and diluted the field - or could even change from a
    >repulsive force to an attractive one, which could set off a
    >big crunch.
    >
    >Recently, in a variation on the quintessence idea, Dr.
    >Leonard Parker of the University of Wisconsin at Milwaukee
    >and various colleagues, including Dr. Caldwell, have
    >suggested that the field associated with some unknown very
    >light particle could get tangled up with gravity and cause
    >the universe to accelerate. That would alter Einstein's
    >equations, said Dr. Caldwell. He added, "Our calculations
    >show, however, that galaxies reside in a bubble of
    >old-fashioned Einstein gravity, whereas gravity has changed
    >outside and between galaxies."
    >
    >A Weird Idea Gets Weirder
    >
    >But the strangest notion is what Dr. Caldwell has called
    >phantom energy, the dark energy that could lead to the Big
    >Rip.
    >
    >"It's weird negative pressure," said Dr. Lawrence M.
    >Krauss, an astrophysicist at Case Western Reserve
    >University in Cleveland.
    >
    >While the density of the energy in Einstein's cosmological
    >constant stays the same as the universe expands, the
    >density of phantom energy would go up and up, eventually
    >becoming infinite. Such would be the case if the parameter
    >w turned out to be less than minus 1, say physicists, who
    >admit they are stunned by the possibility and until
    >recently simply refused to consider it.
    >
    >"It crosses a boundary of good taste," Dr. Caldwell said,
    >calling phantom energy "bad news stuff." Phantom energy
    >violates physicists' intuitions about how the universe
    >should behave. A chunk of it could be used to prop open
    >wormholes in space and time - and thus create time
    >machines, for example.
    >
    >"It could lead to such bizarre effects as negative kinetic
    >energy," Dr. Krauss said. As a result, objects like atoms
    >would be able to lose energy by speeding up.
    >
    >Nevertheless, a recent analysis by Dr. Caldwell and his
    >Dartmouth colleague Dr. Michael Doran of the supernova
    >measurements to date, combined with other cosmological
    >data, suggest that w could lie anywhere from minus 0.8 to
    >minus 1.25, leaving open the possibility of phantom energy.
    >The cosmological constant would give a value of minus 1.0,
    >and anything higher would be a sign of quintessence.
    >
    >Dr. Kirshner said phantom energy had been dismissed as "too
    >strange" when his group was doing calculations of dark
    >energy back in 1998. In retrospect, he said, that was not
    >the right thing to do.
    >
    >"It sounds wacky," he said, referring to phantom energy,
    >"but I think we're in a situation where we're going to need
    >a really new idea. We're in trouble; the way out is going
    >to be new imaginative things. It might be our ideas are not
    >wild enough, they don't question fundamentals enough."
    >
    >Dr. Chris Pritchet of the University of Victoria, who is
    >part of a collaboration using the Canada-France-Hawaii
    >telescope on Mauna Kea to search for supernovas, said, "In
    >many ways phantom energy is unphysical, but we're not
    >ruling it out."
    >
    >Counting Down to the Big Rip
    >
    >This version of doomsday would start slowly. Then, billions
    >of years from now, as phantom energy increased its push and
    >the cosmic expansion accelerated, more and more galaxies
    >would start to disappear from the sky as their speeds
    >reached the speed of light.
    >
    >But things would not stop there. Some billions of years
    >from now, depending on the exact value of w, the phantom
    >force from the phantom energy will be enough to overcome
    >gravity and break up clusters of galaxies. That will happen
    >about a billion years before the Big Rip itself.
    >
    >After that the apocalypse speeds up. About 900 million
    >years later, about 60 million years before the end, our own
    >Milky Way galaxy will be torn apart. Three months before
    >the rip, the solar system will fly apart. The Earth will
    >explode when there is half an hour left on the cosmic
    >clock.
    >
    >The last item on Dr. Caldwell's doomsday agenda is the
    >dissolution of atoms, 10-19, a tenth of a billionth of a
    >billionth of a second before the Big Rip ends everything.
    >
    >"After the rip is like before the Big Bang," Dr. Caldwell
    >said. "General relativity says: "The end. Time can't
    >evolve."
    >
    >The cosmos probably still has a lot of life in it,
    >according to recent calculations by Dr. Krauss. Based on
    >the current age of the universe, some 14 billion years, and
    >other data, w cannot be less than about minus 1.2, he said,
    >putting the Big Rip about 55 billion years in the future.
    >
    >"It can't be very phantom," Dr. Krauss said.
    >
    >The dark
    >energy surveys now under way hope to be able to measure w
    >to an accuracy of 5 percent, but even if that can be done,
    >it may not be sufficient to eliminate the nightmare of
    >phantom energy.
    >
    >"It's hard to measure anything in astronomy to a few
    >percent," said Dr. Sandra Faber of the University of
    >California at Santa Cruz, who directs one of the dark
    >energy surveys. Variations in the atmosphere and gaps in
    >astronomers' understanding of supernova explosions add
    >uncertainty to the dark energy measurements.
    >
    >As a result some astronomers fear that the results may
    >leave us on the razor's edge unable to decide between a
    >cosmological constant and the other possibilities -
    >quintessence or a Big Rip. Cosmologists could then be stuck
    >with a "standard model" of the universe that fits all the
    >data, but which they have no hope of understanding.
    >
    >If the parameter w comes out to be something other than
    >minus 1, Dr. Krauss said, it will at least give some
    >direction to physicists.
    >
    >One encouraging sign - "a tantalizing bit of hope," in Dr.
    >Krauss's words - that the data will distinguish between a
    >cosmological constant and the other possibilities came last
    >fall when Dr. Riess, of Baltimore, reported, based on new
    >observations of distant supernovas, that the "cosmic jerk"
    >when dark energy took over the universe happened only five
    >billion years ago.
    >
    >In the standard cosmological constant model, said Dr.
    >Riess, the turnaround should have come one or two billion
    >years earlier.
    >
    >Dr. Tyson was more sanguine. "Dark energy is crazy, right?"
    >he said. "It's going to be exciting no matter what we
    >find."
    >
    >Dark Future for Dark Energy?
    >
    >The work of the dark energy hunters has been complicated by
    >the impending loss of the Hubble Space Telescope, which can
    >see far enough out in space and time to measure how and if
    >the dark energy parameter w is changing over the eons.
    >
    >Last month, citing safety, NASA canceled all future shuttle
    >maintenance missions to the telescope, dooming it to die in
    >orbit, probably within three years, according to
    >astronomers. "The Hubble shutdown will slow us all down,"
    >Dr. Perlmutter said.
    >
    >At the same time, as a result of the agency's
    >presidentially ordered shift toward the Moon and Mars,
    >plans for a special satellite that was to have been jointly
    >sponsored by NASA and the Department of Energy have at
    >least temporarily disappeared from NASA's five-year budget
    >plan.
    >
    >Dr. Perlmutter, who has devoted much of his time in the
    >last six years to the proposed satellite experiment, said
    >he hoped that a way would be found to keep the project on
    >track to be launched in the next decade.
    >
    >"When you have the most exciting scientific problem of the
    >day, you don't want to wait around," he said.
    >
    >http://www.nytimes.com/2004/02/17/science/space/17DARK.html?ex=1078023766&ei=1&en=ba66bb02e261b870
    >
    >

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