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In the present paper, we numerically construct new non-topological, spontaneously scalarized neutron stars in the tensor-multi-scalar theories of gravity whose target space is a three-dimensional maximally symmetric space, namely either $\mathbb{S}^3$, $\mathbb{H}^3$ or $\mathbb{R}^3$, and in the case of a nontrivial map $\varphi : \text{\it spacetime} \to \text{\it target space}$.
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D. D. Doneva and S. S. Yazadjiev, arXiv:1909.00473 [gr-qc]
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D. D. Doneva and S. S. Yazadjiev, arXiv:1911.06908 [gr-qc]
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2015
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D. Doneva and S. Yazadjiev, Phys. Rev. Lett. 120 (2018) no.13, 131103 [arXiv:1711.01187 [gr-qc]]
2018
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2018
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D. D. Doneva and S. S. Yazadjiev, JCAP 1804
2018
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