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                                                                                            A Closer Look


                                                                                                           Dark Energy
                             he first evidence came from astron-  By comparing these two light sources,   as a function of space. This means there
                          Tomers trying to measure how fast   astronomers would be able to calculate   was not much—shall we say, dark energy—
                          the  expanding universe is slowing. At the   the expansion rate for now and in the dis-  when the universe was smaller, and grav-
                          time, the generally accepted model of the   tant past.                ity slowed the expansion. As the distance
                          universe was that it was still expanding   To their surprise, the astronomers did   between galaxies increased, there was an
                          but had been slowing from gravitational   not find a rate of slowing expansion. Rather,   increase of dark energy, and the expan-
                          attraction since the big bang. The astrono-  they found that the expansion is speed-  sion accelerated. Einstein removed this
                          mers intended to measure the slowing rate   ing up. There was no explanation for this   constant when Edwin Hubble reported
                          to determine the average density of matter   speeding up other than to assume that some   evidence that the universe is expanding.
                          in the universe, providing a clue about the   unknown antigravity force was at work.   Removing the constant may have been a
                          extent of dark matter. Their idea was to   This unknown force must be pushing the   mistake. One of the problems in under-
                          compare light traveling from a supernova   galaxies farther apart at the same time that   standing what was happening to the early
                          in the distant universe with light traveling   gravity is trying to pull them together. The   universe compared to now was a lack of
                          from a much closer supernova. Light from   unknown repulsive force became known as   information about the past as represented
                          the distant universe is just now reaching   “dark energy.”            by the distant, faraway universe. Today,
                          us because it was emitted when the uni-  The idea of an unknown repulsive   this is changing as more new technology
                          verse was very young. The brightness of   force is not new. It was a new idea when   is helping astronomers study the faraway
                          the older and younger supernova would   Einstein added a “cosmological constant”   universe. Will they find the meaning
                          provide information about distance, and   to the equations in the theory of general   of dark energy? What  is dark energy?
                          expansive redshift data would provide in-  relativity. This constant represents a force   The answer is that no one knows. Stay
                          formation about their speed of expansion.   that opposes gravity, and the force grows   tuned . . . this story will be continued.






                       to their distance away. It would not matter which raisin you were   tinuing. All the evidence tells us it began by expanding with a
                       on since all the raisins would appear to be moving away to all the   big bang. Will it continue to expand, becoming increasingly
                       other raisins. In other words, the galaxies are not expanding into   cold and diffuse? Will it slow to a halt, then start to contract to a
                       space that is already there. It is space itself that is expanding, and   fiery  finale of a big crunch (Figure 14.19)? Researchers continue
                       the galaxies move with the expanding space (Figure 14.18).  searching for answers with experimental data and theoreti-
                           The ultimate fate of the universe will strongly depend on   cal models, looking for clues in matches between the data and
                       the mass of the universe and if the expansion is slowing or con-  models.































                       FIGURE 14.18  Will the universe continue expanding as the dust and gas in galaxies become locked up in white dwarf stars, neutron stars,
                       and black holes?

                        14-17                                                                       CHAPTER 14  The Universe   367
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