ar X iv : h ep - p h / 97 10 56 2 v 1 3 1 O ct 1 99 7 1260 : Phenomenology of Antigravity in N = , Supergravity

نویسنده

  • Stefano Bellucci
چکیده

N = 2, 8 supergravity predicts antigravity (gravivector and graviscalar) fields in the graviton supermultiplet. Data on the binary pulsar PSR 1913+16, tests of the equivalence principle and searches for a fifth force yield an upper bound of order 1 meter (respectively, 100 meters) on the range of the gravivector (respectively, graviscalar) interaction. Hence these fields are not important in non-relativistic astrophysics (for the weak-field limit of N = 2, 8 supergravity) but can play a role near black holes and for primordial structures in the early universe of a size comparable to their Compton wavelengths. The quest for a unified description of elementary particle and gravity theories led to local supersymmetry [1]. The large symmetry content of supergravity yields, in spite of its lack of renormalizability, powerful constraints on physical observables, e.g. anomalous magnetic moments [2]. It has been shown that a clear case for antigravity theories arises, when considering N > 1 supergravity theories [3, 4]. Combining laboratory data together with geophysical and astronomical observations has provided us restrictions on the antigravity features of some extended supergravity theories [5, 6]. This can have important consequences for high precision experiments measuring the difference in the gravitational acceleration of the proton and the antiproton [7]. A review of earlier ideas about antigravity is found in [8]. The N = 2, 8 supergravity multiplets contain, in addition to the graviton, a vector field A l µ [9], [10, 11]. This field, which we refer to as the gravivector, carries antigravity, because it couples to quarks and leptons with a positive sign and to antiquark and antileptons with a negative one. The coupling is proportional to the mass of the matter fields and vanishes for self-conjugated particles. The other antigravity field is the scalar σ entering the N = 8 supergravity multiplet [3, 4]. We refer to it as the graviscalar. We are bound, in force of the result of the Eötvös experiment, to take a nonvanishing mass for the field A l µ [3, 4]. m l = 1 R l = 4πG N m φ φ , m φ = φ , (1) where the Higgs mechanism has been invoked. The presence of the gravivector in the theory introduces a violation of the equivalence principle on a range of distances of order the Compton wavelength R l. At present, the equivalence principle is verified with a precision |δγ/γ| <

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ar X iv : h ep - p h / 96 05 44 3 v 1 3 0 M ay 1 99 6 Effects of the gravivector and graviscalar fields in N = 2 , 8 supergravity ∗

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تاریخ انتشار 1997