Why Is The Universe Expanding?

Einstein believed that the Universe was an infinitely large, all-encompassing blimp. His General Theory of Relativity suggested a model of a Universe that was homogenous, spatially curved and dominated by a single force – gravity. However, if gravity alone sculpts the structure of the Cosmos, then all matter in it must be impelled to be mutually attracted towards each other rendering the Universe to crumble under its own weight.

Clearly, this is not the case. To account for the Universe’s apparent stability, Einstein included a constant in his equations, a constant that would neutralize the inexorable pull of gravity. He called this the cosmological constant. The resulting Universe was a place that neither contracted nor expanded. This was Einstein’s infamous static Universe.

Albert Einstein during a lecture in Vienna in 1921

Albert Einstein (Photo Credit: Ferdinand Schmutzer / Wikipedia Commons)

Red Shift

As it turns out, he was wrong, albeit not entirely. There’s an old legend according to which Einstein discarded his static Universe after Hubble observed that our neighboring galaxies are moving away from us. Hubble witnessed how the wavelengths of light emitted by these galaxies were stretched and elongated as they moved further from us, a phenomenon known as red-shifting.

The truth, however, is a bit more complex. Before Hubble’s revolutionary discovery, based on the dissonance in various astronomical observations and his equations, Einstein was prodded by several of the most brilliant astrophysicists of his generation to modify his current model. Obstinate, he adopted an expanding Universe theory after nearly 14 years.

However, not only is the Universe expanding, but its expansion is accelerating. This means that galaxies further away from us are receding at a much faster velocity than galaxies nearer to us. So… what mysterious force is driving this extraordinary expansion?

Dark Energy

Hubble’s discovery is one of mankind’s seminal discoveries. The expansion implies that there are not one, but two, large-scale forces dominating the structure of the Universe – the inward pulling force of gravity and the mysterious repulsive force that is shoving matter apart. Currently, the rate of expansion – or Hubble’s constant – is calculated to be 44.7 miles per second per megaparsec (one parsec is just over three light years). This value suggests that the distance between cosmic objects will double in another 9.8 billion years!

milky way galaxy

The Milky Way (Photo Credit: passmil198216 / Fotolia)

However, while gravity is an attractive force that works on objects, the repulsive force works on space instead. The distribution of chocolate chips on a brittle cookie provides a good analogy to understand these forces of nature. If the cookie represents all the space in the Universe and the chocolate chips are its galaxies, then gravity is a force that impels every chip to move towards every other chip, whereas the repulsive force expands the cookie itself. Despite being in the same place, the chips appear to be vastly separated due to the extension of the cookie-space between them.

Mysterious is a fitting term to describe this force. Cosmologists refer to it as Dark Energy. The most perplexing characteristic of this energy is its source. Einstein’s most famous equation, the one people most immediately associate with him, E = MC², showed that mass and energy are interchangeable, that they are different forms of the same entity. It is the conversion of mass into energy inside the Sun’s core that fuels its copious radiation.

But what about dark energy? Its work on space or vacuum implies that space harbors an enormous amount of energy, even when it’s devoid of all matter or radiation. How is this possible? Some speculate that vacuum isn’t empty, but rather teeming with particles that incessantly pop in and out of absolutely nowhere. Apparently, quantum mechanics allows this (why am I not surprised). It may be this constant boiling that so powerfully energizes space.

quantum entanglement

Some speculate that vacuum isn’t empty, but rather teeming with particles that incessantly pop in-and-out of absolutely nothing. Credits:MichaelTaylor/Shutterstock

Or, it could be an exotic new force that eludes detection, perhaps because our understanding of the absurd laws of the Universe is incomplete. Currently, dark energy is believed to be the personification of Einstein’s cosmological constant, which is why he was wrong, albeit not entirely. The notion of dark energy is particularly terrifying because it constitutes almost 70% — an indomitable majority — of all the energy fostered by the Universe. Only 4% is visible matter! Basically, we have no clue what our Universe is made of.

The Repulsive Conclusion

The Cosmic Microwave Background Radiation (CMBR) is an almost uniform background of microwaves spread across the entire Universe. It is the leftover heat from the Big Bang and paints the entire sky. It is also the oldest light we can see. The CMBR provides us with a picture of the infant Universe, almost 100,000 years after its birth.

CMBR is the leftover heat from the Big Bang and paints the whole sky. It is also the oldest light we can see.(PhCredit:it : AirBa~commonswiki / Wikimedia Commons)

The CMBR, an indelible proof of the Big Bang, also gives us insight on how the Universe might end. The tiny differences in temperature, and thus density, help cosmologists determine the shape of the Universe. For instance, if the shape of the Universe was ‘closed’, then at some point the expansion would eventually be triumphed by contraction, causing the Universe to gradually collapse into itself. On the other hand, if it was ‘open’, the Universe would keep expanding forever.

shape of universe End of universe

Shape of Universe where Ω is the density parameter (Credits:NASA/Wikipedia)

However, the shape of our Universe, as the CMBR limned, was ‘flat’. It initially expanded at a blistering rate, but the rate of expansion eventually slowed down. This profound discovery, however, entails a repulsive conclusion. Currently, the Universe and modern cosmology are in their honeymoon phase; the expansion has neither driven the neighboring galaxies too far to be out of our reach, nor are they too close to render us incapable of discerning any vital difference.

Stars in the sky

The stars could not have aligned in a better way. (Photo Credit: Pixabay)

If the expansion continues at this rate, our neighboring galaxies will soon recede to the extent that cosmological equipment would be no more useful than a scissor with one blade. The expansion would elongate and eventually completely placate the CMBR as well. This would render subsequent generations oblivious to the occurrence of the Big Bang. Cosmologists look forward to making the best of these times and accrue as much data as this era of expansion bestows. The stars could not have aligned in a better way!

References

  1. Phys.org
  2. Hubblesite.org
  3. Library of Congress
  4. Wikipedia
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About the Author:

Akash Peshin is an Electronic Engineer from the University of Mumbai, India and a science writer at ScienceABC. Enamored with science ever since discovering a picture book about Saturn at the age of 7, he believes that what fundamentally fuels this passion is his curiosity and appetite for wonder.

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