ℓ-boson stars

By M. Alcubierre, J. Barranco, A. Bernal, J. C. Degollado, A. Diez-Tejedor, M. Megevand, D. Núñez, O. Sarbach. Classical and quantum gravity, 2018

177 citations recorded by the source corpus.

We present new, fully nonlinear numerical solutions to the static, spherically symmetric Einstein–Klein–Gordon system for a collection of an arbitrary odd number N of complex scalar fields with an internal symmetry and no self-interactions. These solutions, which we dub -boson stars, are parametrized by an angular momentum number , an excitation number n, and a continuous parameter representing the amplitude of the fields. They are regular at every point and possess a finite total mass. For the standard spherically symmetric boson stars are recovered. We determine their generalizations for , and show that they give rise to a large class of new static configurations which might have a much larger compactness ratio than stars.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/03e040702ffd9ed259c5eb05232bc228bcbf97b0

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In Astronomy and Astrophysics

  1. Diego Rubiera-García
  2. Aneta Wojnar
  3. Eran Palti
  4. Farvah Mahmoudi
  5. A. Arbey
  6. G. Olmo
  7. Valerio Faraoni
  8. Tiberiu Harko

In Nuclear and High Energy Physics

  1. Diego Rubiera-García
  2. Aneta Wojnar
  3. A. Arbey
  4. Eran Palti
  5. Farvah Mahmoudi
  6. G. Olmo
  7. Valerio Faraoni
  8. Tiberiu Harko

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