The Big Bang Theory (Edexcel IGCSE Physics (Modular))

The Big Bang theory

• Around 14 billion years ago, the Universe began from a very small region that was extremely hot and dense

• Then there was a giant explosion, which is known as the Big Bang

• This caused the universe to expand from a single point, cooling as it does so, to form the universe today

• Each point expands away from the others

  • This is seen from galaxies moving away from each other, and the further away they are the faster they move

• As a result of the initial explosion, the Universe continues to expand

All galaxies are moving away from each other, indicating that the universe is expanding

• An analogy of this is points drawn on a balloon where the balloon represents space and the points as galaxies

• When the balloon is deflated, all the points are close together and an equal distance apart

• As the balloon expands, all the points become further apart by the same amount

• This is because the space itself has expanded between the galaxies

  • Therefore, the density of galaxies falls as the Universe expands

A balloon inflating is similar to the stretching of the space between galaxies

Evidence for the Big Bang

What are two pieces of evidence that support the Big Bang theory?

• Since there is more evidence supporting the Big Bang theory than the Steady State theory, it is the currently accepted model for the origin of the Universe

• The two main pieces of evidence supporting the Big Bang are

  • Galactic red-shift

  • Cosmic Microwave Background (CMB) radiation

Evidence from galactic red-shift

• By observing the light spectrums from supernovae in other galaxies there is evidence to suggest that distant galaxies are receding (moving further apart) even faster than nearby galaxies

  • These observations were first made in 1998

• The light spectrums show that light from distant galaxies is redshifted, which is evidence that the universe is expanding

• As a result, astronomers have concluded that:

  • All galaxies are moving away from the Earth

  • Galaxies are moving away from each other

• This is what is expected after an explosion

  • Matter is first densely packed and as it explodes it, it moves out in all directions getting further and further from the source of the explosion

  • Some matter will be lighter and travel at a greater speed, further from the source of the explosion

  • Some matter will be heavier and travel at a slower speed, closer to the source of the explosion

• If someone were to travel back in time and compare the separation distance of the galaxies:

  • It would be seen that galaxies would become closer and closer together until the entire universe was a single point

• If the galaxies were originally all grouped together at a single point and were then exploded a similar effect would be observed

  • The galaxies that are the furthest are moving the fastest - their distance is proportional to their speed

  • The galaxies that are closer are moving slower

Tracing the expansion of the universe back to the beginning of time leads to the idea the universe began with a “big bang”

Evidence from CMB radiation

• The discovery of the CMB (Cosmic Microwave Background) led to the Big Bang theory becoming the currently accepted model

  • The CMB is a type of electromagnetic radiation which is a remnant from the early stages of the Universe

  • It has a wavelength of around 1 mm making it a microwave, hence the name Cosmic Microwave Background

• In 1964, Astronomers discovered radiation in the microwave region of the electromagnetic spectrum coming from all directions and at a generally uniform temperature of 2.73 K

  • They were unable to do this any earlier since microwaves are absorbed by the atmosphere

  • Around this time, space flight was developed which enabled astronomers to send telescopes into orbit above the atmosphere

• According to the Big Bang theory, the early Universe was an extremely hot and dense environment

  • As a result of this, it must have emitted thermal radiation

• The radiation is in the microwave region

  • This is because over the past 14 billion years or so, the radiation initially from the Big Bang has become redshifted as the Universe has expanded

  • Initially, this would have been high energy radiation, towards the gamma end of the spectrum

  • As the Universe expanded, the wavelength of the radiation increased

  • Over time, it has increased so much that it is now in the microwave region of the spectrum

The CMB is a result of high energy radiation being redshifted over billions of years

• The CMB radiation is very uniform and has the exact profile expected to be emitted from a hot body that has cooled down over a very long time

  • This phenomenon is something that other theories (such as the Steady State Theory) cannot explain

• The CMB is represented by the following map:

The CMB map with areas of higher and lower temperature. Places with higher temperature have a higher concentration of galaxies, Suns and planets

• This is the closest image to a map of the Universe

• The different colours represent different temperatures

  • The red / orange / brown regions represent warmer temperature indicating a higher density of galaxies

  • The blue regions represents cooler temperature indicating a lower density of galaxies

• The temperature of the CMB is mostly uniform, however, there are minuscule temperature fluctuations (on the order of 0.00001 K)

  • This implies that all objects in the Universe are more or less uniformly spread out