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单词 big-bang theory
释义
big-bang theory

Physics
  • Newton’s work gave a mathematical basis for the universe on a large scale. However, the data available at the time suggested a static unchanging universe. This could not easily be explained in the context of the law of gravitation, since all bodies in the universe attract all other bodies with the force of gravity. Newton realized that there was only one solution to this problem: in a static universe, matter had to be uniformly spread throughout an infinitely large space. In 1826, Heinrich Olbers published a paper containing what is known as Olbers’ paradox; such a universe would lead to a perpetually bright sky on earth.

    Space–time

    Cosmologists now believe that Newton’s model was based on incorrect assumptions about the structure of space, time, and matter. Einstein in his general theory of relativity (1915) proposed that the universe exists in four-dimensional space–time. This space–time is curved by the presence of matter, and the matter moves by following the resulting curves.

    The expanding universe

    The discovery by Hubble in 1929 that the universe is expanding provided a starting point for the ideas on which our present understanding of the universe is based. Hubble made his discovery by analysing the spectra of light from distant galaxies and noting a persistent redshift, which he explained in terms of the Doppler effect; an increase in observed wavelengths of light occurs because the light source is receding from the observer. The larger the speed of recession, the larger the red shifts. Hubble discovered a pattern in his data: the further away the galaxy, the greater the speed of recession. Known as Hubble’s law, this provided the evidence that the universe is expanding and a resolution to Olbers’ paradox. If the galaxies and the earth are moving apart, the radiation falling on the earth from the galaxies is reduced. The further galaxies are away from the earth, the smaller their contribution to the radiation falling on the earth.

    This model might seem to place the earth at the centre of the universe again. However, it is space itself that is expanding and the galaxies are imbedded in this space. The ring (space) in the diagram has dots (the galaxies). The expansion of the ring means that the view from any one dot is that the other dots are receding at a speed proportional to their distance away. No single dot is at the centre of the system but all dots see the same thing.

    Age of the universe

    Hubble’s law may be stated in the form H0=v/d, where v is the speed of recession of the galaxy, d is the earth–galaxy distance, and H0 is called the Hubble constant. Assuming that the galaxies have always been moving apart, the age of the universe (T) can be estimated, i.e. T=1/H0. On this basis and from other considerations the age of the universe would be about 13.8 billion years.

    big-bang theory

    The expansion leads to the recession of B from A along the ring. The speed of recession will be directly proportional to the distance of B from A along the ring.

    The origin of the universe

    This view of the origin of the universe is called the big-bang theory, first put forward by Georges Lemaître in 1927. The theory suggests that the universe originated as a minute but very hot body and that the temperature has been falling as the expansion has continued. In several papers in the 1940s Ralph Alpher and Robert Herman working with George Gamow predicted that there should be a microwave background corresponding to a black-body temperature a few degrees above absolute zero. This microwave background was discovered 20 years later. The big-bang theory also explains the amount of helium in the universe.

    In 1992, the COBE satellite discovered that there were very small variations in the microwave background. This discovery helped to explain why the universe formed into galaxies and stars. The nonuniformities that began the nucleation of galactic matter in the early universe now appear as the small variations in the microwave background. In 1998 it was discovered that the expansion of the universe is accelerating.

    Fundamental forces

    It is thought that the four fundamental interactions in the universe are all manifestations of the same force. This force existed when the big bang occurred at a temperature above 1015K. As the universe cooled the forces separated as the original symmetries were broken. Gravity was the first to separate, followed by the strong nuclear force, and the weak and electromagnetic forces (see table).

    Time from big bang

    Temperature (K)

    State of the universe/forces

    0 second

    infinite

    The universe is infinitesimally small and infinitely dense (i.e. a mathematical singularity).

    10−12 second

    1015

    Weak and electromagnetic forces begin to separate.

    10−6 second

    1014

    Quarks and leptons begin to form.

    10−3 second

    1012

    Quarks form the hadrons; quark confinement begins.

    102 second

    107

    Helium nuclei formed by fusion.

    105 years

    104

    Atomic era; atoms form as protons combine with electrons.

    106 years

    103

    Matter undergoes gravitational collapse.

    1.8 × 1010 years

    2.7

    Present day: cosmic background corresponds to about 2.7K.

    The future

    Research into the future of the universe is clearly speculative. Whether the universe will continue to expand indefinitely depends on its mean density. Below a critical level (the critical density), gravitational attraction will not be enough to stop the expansion. However, if the mean density is above the critical density the universe is bound and an eventual contraction will occur, resulting in a big crunch. This may precede another big bang, initiating the whole cycle again. However, the discovery that the expansion of the universe is accelerating makes the big crunch a much less likely scenario.


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