l-boson stars

被引:60
作者
Alcubierre, Miguel [1 ]
Barranco, Juan [2 ]
Bernal, Argelia [2 ]
Carlos Degollado, Juan [3 ]
Diez-Tejedor, Alberto [2 ]
Megevand, Miguel [4 ]
Nunez, Dario [1 ]
Sarbach, Olivier [5 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, Circuito Exterior CU,AP 70-543, Mexico City 04510, DF, Mexico
[2] Univ Guanajuato, Dept Fis, Div Ciencias & Ingn, Campus Leon, Leon 37150, Mexico
[3] Univ Nacl Autonoma Mexico, Inst Ciencias Fis, Apdo Postal 48-3, Cuernavaca 62251, Morelos, Mexico
[4] Consejo Nacl Invest Cient & Tecn, Inst Fis Enrique Gaviola, Ciudad Univ, RA-5000 Cordoba, Argentina
[5] Univ Michoacana, Inst Fis & Matemat, Edificio C-3,Ciudad Univ, Morelia 58040, Michoacan, Mexico
关键词
boson stars; classical general relativity; compact objects; STABILITY;
D O I
10.1088/1361-6382/aadcb6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 U(N) symmetry and no self-interactions. These solutions, which we dub l-boson stars, are parametrized by an angular momentum number l = ( N - 1)/2, 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 l= 0 the standard spherically symmetric boson stars are recovered. We determine their generalizations for l > 0, and show that they give rise to a large class of new static configurations which might have a much larger compactness ratio than l = 0 stars.
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页数:13
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共 29 条
[1]   Constraining scalar fields with stellar kinematics and collisional dark matter [J].
Amaro-Seoane, Pau ;
Barranco, Juan ;
Bernal, Argelia ;
Rezzolla, Luciano .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2010, (11)
[2]   Bosonic gas as a galactic dark matter halo [J].
Arturo Urena-Lopez, L. ;
Bernal, Argelia .
PHYSICAL REVIEW D, 2010, 82 (12)
[3]   Self-gravitating system made of axions [J].
Barranco, J. ;
Bernal, A. .
PHYSICAL REVIEW D, 2011, 83 (04)
[4]   Multistate boson stars [J].
Bernal, A. ;
Barranco, J. ;
Alic, D. ;
Palenzuela, C. .
PHYSICAL REVIEW D, 2010, 81 (04)
[5]   On existence of mini-boson stars [J].
Bizon, P ;
Wasserman, A .
COMMUNICATIONS IN MATHEMATICAL PHYSICS, 2000, 215 (02) :357-373
[6]   Linear perturbations of self-gravitating spherically symmetric configurations [J].
Chaverra, Eliana ;
Ortiz, Nestor ;
Sarbach, Olivier .
PHYSICAL REVIEW D, 2013, 87 (04)
[7]   BOSON STARS - GRAVITATIONAL EQUILIBRIA OF SELF-INTERACTING SCALAR FIELDS [J].
COLPI, M ;
SHAPIRO, SL ;
WASSERMAN, I .
PHYSICAL REVIEW LETTERS, 1986, 57 (20) :2485-2488
[8]   COMMENTS ON NONLINEAR WAVE EQUATIONS AS MODELS FOR ELEMENTARY PARTICLES [J].
DERRICK, GH .
JOURNAL OF MATHEMATICAL PHYSICS, 1964, 5 (09) :1252-&
[9]   No-go theorem for static scalar field dark matter halos with no Noether charges [J].
Diez-Tejedor, Alberto ;
Gonzalez-Morales, Alma X. .
PHYSICAL REVIEW D, 2013, 88 (06)
[10]   MINI-SOLITON STARS [J].
FRIEDBERG, R ;
LEE, TD ;
PANG, Y .
PHYSICAL REVIEW D, 1987, 35 (12) :3640-3657