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Exact Solutions and Scalar Fields in Gravity - Instituto Avanzado de ...

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108 EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY<br />

The value of the parameter is the same as <strong>in</strong> (24). The<br />

cosmological function orig<strong>in</strong>ated by the Higgs-potential is necessarily<br />

positive <strong>and</strong> possesses the value:<br />

It vanishes for the ground–state The first bracket on the right<br />

h<strong>and</strong> si<strong>de</strong> of (36) represents the effective energy–momentum tensor of<br />

fermions <strong>and</strong> gauge bosons tak<strong>in</strong>g additionally <strong>in</strong>to account the masses<br />

of the gauge bosons <strong>and</strong> energy <strong>and</strong> momentum of the excited Higgs–<br />

field.<br />

In the same way it follows from (29) after <strong>in</strong>sertion of (37) <strong>and</strong> (23)<br />

with the square of the Higgs–mass:<br />

Accord<strong>in</strong>gly the value of (41) is smaller than the usual one (see (21)) by<br />

the very small factor <strong>and</strong> of the same or<strong>de</strong>r of magnitu<strong>de</strong> as see<br />

(39). In consequence of the non-m<strong>in</strong>imal coupl<strong>in</strong>g of the gravitational<br />

<strong>and</strong> the Higgs field <strong>in</strong> (25), the trace T appears as an additional source<br />

<strong>in</strong> (40, which results later <strong>in</strong> a total cancellation of the right h<strong>and</strong> si<strong>de</strong>.<br />

F<strong>in</strong>ally we give the Dirac equation (30) <strong>and</strong> the Yang–Mills equation<br />

(31) after symmetry break<strong>in</strong>g. One obta<strong>in</strong>s with (19)<br />

<strong>and</strong> with (20)<br />

Now we are able to calculate the source of the excited Higgs-field<br />

accord<strong>in</strong>g to (40). From (33) <strong>and</strong> (42) we get for the trace of

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