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and Cosmology

Extragalactic Astronomy and Cosmology: An Introduction

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8. <strong>Cosmology</strong> III: The Cosmological Parameters<br />

354<br />

cessful theory describing dark energy will necessitate<br />

a significant breakthrough in our general underst<strong>and</strong>ing<br />

of fundamental physics.<br />

The search for the constituents of dark matter will<br />

keep physicists busy in the coming years. Experiments<br />

at future particle accelerators (e.g., the LHC at CERN)<br />

<strong>and</strong> the direct search, in underground laboratories, for<br />

particles which may account for c<strong>and</strong>idates of dark matter,<br />

are promising. In any case, dark matter (if it indeed<br />

consists of elementary particles) will open up a new<br />

field in particle physics. For these reasons, the interests<br />

of cosmology <strong>and</strong> particle physics are increasingly converging<br />

– in particular since the Universe is the largest<br />

<strong>and</strong> cheapest laboratory for particle physics.

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