Gravitational mass-shift effect in the standard model

P. O. Kazinski

Результат исследований: Материалы для журналаСтатья

7 Цитирования (Scopus)


The gravitational mass-shift effect is investigated in the framework of the standard model with the energy cutoff regularization both for stationary and nonstationary backgrounds at the one-loop level. The problem of singularity of the effective potential of the Higgs field on the horizon of a black hole, which was reported earlier, is resolved. The equations characterizing the properties of a vacuum state are derived and solved in a certain approximation for the Schwarzschild black hole. The gravitational mass-shift effect is completely described in this case. The behavior of masses of the massive particles of the standard model depends on the value of the Higgs boson mass in a flat spacetime. If the Higgs boson mass in a flat spacetime is less than 263.6 GeV then a mass of any massive particle approaching a gravitating object grows. If the Higgs boson mass in a flat spacetime is greater than or equal to 278.2 GeV, the masses of all the massive particles decrease in a strong gravitational field. The Higgs boson masses lying between these two values prove to lead to instability, at least at the one-loop level, and so they are excluded. It turns out that the vacuum possesses the same properties as an ultrarelativistic fluid in a certain approximation. The expression for the entropy and enthalpy densities and the pressure of this fluid are obtained. The sound speed in this fluid is also derived.

Язык оригиналаАнглийский
Номер статьи044008
ЖурналPhysical Review D - Particles, Fields, Gravitation and Cosmology
Номер выпуска4
СостояниеОпубликовано - 6 фев 2012
Опубликовано для внешнего пользованияДа

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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