How Will the Universe End?

     

    In 1929, Edwin Hubble discovered that the universe is not in fact static, but expanding. In the years following his discovery, cosmologists took up the implications of the discovery, asking how long the universe had been expanding, what forces caused the expansion, and whether it will ever cease. 

      

   Cosmologists are pretty confident about the first question: just shy of 14 billion years. A great deal of evidence supports the predominant answer to the second question: The universe rapidly emerged from  a  singularity  in  an  event  that cosmologists call the Big Bang. The third question is a bit more mysterious, and the answer relies on an obscure, confounding phenomenon known as dark energy. The density of dark energy in the universe determines  its  ultimate  fate.  In  one scenario, the universe does not possess enough dark energy to forever counteract its own gravity and thus ends in a "Big Crunch."  Under  this  scenario,  the universe's gravity will overcome its expansion and the cosmos will collapse in on itself, resulting in a singularity that may precipitate another Big Bang. However, the evidence cosmologists have gathered over the last few decades leads us away from this scenario.

      

    For the Big Crunch to occur, we'd see signs that gravity was winning out over dark  energy,  slowing  its  expansion. However, measurements of distant galaxies indicate that cosmic expansion is not slowing   down-it's   speeding   up! Apparently, the density of dark energy in the vacuum of space is simply too high to permit a Big Crunch. That leaves two possible fates for the cosmos: 1) a Big Freeze, in which the acceleration  eventually  halts  but  the universe  keeps  expanding,  creating  a system  where  heat  becomes  evenly distributed, allowing no room for usable energy to exist and thus, "heat death," or 2) a Big Rip, in which the expansion of the universe continues to accelerate forever. In  the former scenario, the universe will  progressively become darker and colder  until the end of time. In the latter, all  matter down to  the  most  fundamental  particles will be torn asunder.    

  

   All the recent data from the Planck  space observatory and the Sloan Digital  Sky Survey suggest there is just enough  dark energy to continue the universe's  expansion, but not enough to keep it  accelerating  forever.  This  conclusion  points toward the Big Freeze, or "heat   death" of the universe. The most up-to-date science leads us to the conclusion that our  universe-and Robert Frost's-is more  likely to end in ice than in fire. That, however, assumes that what we believe about dark energy is true. Considering that dark energy itself is a phenomenon cloaked deeply in mystery, such assumptions may yet prove untenable.