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

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A plane–fronted wave solution <strong>in</strong> metric–aff<strong>in</strong>e gravity 143<br />

<strong>and</strong> of the canonical energy–momentum, the metric stress–energy, <strong>and</strong><br />

the hypermomentum current of the gauge fields,<br />

Moreover, we <strong>in</strong>troduced the canonical energy–momentum, the metric<br />

stress–energy, <strong>and</strong> the hypermomentum currents of the matter fields,<br />

respectively,<br />

Provi<strong>de</strong>d the matter equation (2) is fulfilled, the follow<strong>in</strong>g Noether i<strong>de</strong>ntities<br />

hold:<br />

They show that the field equation (3) is redundant. Thus we only need<br />

to take <strong>in</strong>to account (4) <strong>and</strong> (5). As suggested <strong>in</strong> [2], the most general<br />

parity conserv<strong>in</strong>g Lagrangian expressed <strong>in</strong> terms of the irreducible pieces<br />

(cf. [2]) of nonmetricity torsion <strong>and</strong> curvature reads<br />

Note that we <strong>de</strong>compose the curvature 2–form <strong>in</strong>to its antisymmetric<br />

<strong>and</strong> symmetric parts, i.e.<br />

rotational stra<strong>in</strong> curvature. The constants enter<strong>in</strong>g eq. (11) are the<br />

cosmological constant the weak <strong>and</strong> strong coupl<strong>in</strong>g constant <strong>and</strong><br />

respectively, <strong>and</strong> the 28 dimensionless parameters

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