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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Relancio, J.J.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0003-1130-3982</subfield>
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  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Phenomenological consequences of a geometry in the cotangent bundle</subfield>
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    <subfield code="c">2020</subfield>
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    <subfield code="a">A deformed relativistic kinematics can be understood within a geometrical framework through a maximally symmetric momentum space. However, when considering this kind of approach, usually one works in a flat spacetime and in a curved momentum space. In this paper, we will discuss a possible generalization to take into account both curvatures and some possible observable effects. We will first explain how to construct a metric in the cotangent bundle in order to have a curved spacetime with a nontrivial geometry in momentum space and the relationship with an action in phase space characterized by a deformed Casimir. Then, we will study within this proposal two different space-time geometries. In the Friedmann-Robertson-Walker universe, we will see the modifications in the geodesics (redshift, luminosity distance, and geodesic expansion) due to a momentum dependence of the metric in the cotangent bundle. Also, we will see that when the spacetime considered is a Schwarzschild black hole, one still has a common horizon for particles with different energies, differently from a Lorentz invariance violation case. However, the surface gravity computed as the peeling off of null geodesics is energy dependent.</subfield>
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    <subfield code="a">Liberati, S.</subfield>
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    <subfield code="1">2004</subfield>
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    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
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    <subfield code="g">101, 6 (2020), 064062 1-15</subfield>
    <subfield code="p">Phys. rev. D</subfield>
    <subfield code="t">Physical Review D</subfield>
    <subfield code="x">2470-0010</subfield>
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