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<p>symmetry of the string, though balancing the quantum anomalies of this tensor.<br/>
* Scalar fields are hypothesized to have caused the high accelerated expansion of the early universe (<a href="page.php?w=Inflation_%28cosmology%29">inflation</a>), helping to solve the <a href="page.php?w=horizon_problem">horizon problem</a> and giving a hypothetical reason for the non-vanishing <a href="page.php?w=cosmological_constant">cosmological constant</a> of cosmology. Massless (i.e. long-ranged) scalar fields in this context are known as <a href="page.php?w=inflaton">inflaton</a>s.</p><p>
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