标题： 脉冲星踢出效应通过自旋-1色超导性 显示英文标题

标题： Pulsar kicks via spin-1 color superconductivity

摘要： 我们提出了一种新的中微子推进机制，可用于中子星，从而导致强烈的速度脉冲，这可以解释观测到的脉冲星双峰速度分布。 由包含A相自旋-1色超导夸克物质的恒星核心自然提供了中微子发射的空间不对称性。 当中子星的核心温度下降到该相变温度以下时，这种中微子推进机制就会启动。 显示英文摘要

摘要： We propose a new neutrino propulsion mechanism for neutron stars which can lead to strong velocity kicks, needed to explain the observed bimodal velocity distribution of pulsars. The spatial asymmetry in the neutrino emission is naturally provided by a stellar core containing spin-1 color-superconducting quark matter in the A phase. The neutrino propulsion mechanism switches on when the stellar core temperature drops below the transition temperature of this phase.