论文标题
紧凑型恒星残余物中的质量分布和“质量差距”
Mass Distribution and "Mass Gap" of Compact Stellar Remnants in Binary Systems
论文作者
论文摘要
在状态方程和观察结果/观察结果的背景下，对中子星（NSS）的最高临界质量进行了审查。然而，最近对重力波和其他研究的观察结果表明，NSS，MNS 〜3/2 m_sun的质量较高。 NS质量达到MNS〜2 m_sun的价值已得到充分理解，其质量价值非常重要，即讨论NS和Black Hole和Black Hole（BH）折叠之间的“质量差距”（“ M-GAP”）。“ M-GAP”存在于NS质量最高的NS和最低的BH Collapsars（Mm-gapapars）（mmm-gap 〜2-2-2-2-5 m_sun）之间。在质量分布中，NSS和BHS的最大群体分别位于MNS = 1.4 m_sun和MBH = 6.7 m_sun。但是，最近的守护结果预测，紧凑的对象填充了“ M-GAP”。在本文中，据报道，妊娠的概念可以解决MPEAK = 6.7 m_sun和“ M-GAP”（MM-GAP〜2-5 M_SUN）的重力质量峰值值的问题。这个概念基于引力与可局部场能的重力相互作用的非中标量表模型。压力性动力学模型显示了一个紧凑的相对论对象的总质量（MQ），该对象充满了半径r* = gmq/c2〜10 km的夸克 - 杜伦等离子体的物质，与“ M-GAP”一致。概念上认为，这种极度致密的物体的总可测量重力质量由物质和场组成，这是由标量调整组件描述的。该模型对于预测“ M-GAP”中的折叠术也很有用。
The highest critical mass of neutron stars (NSs) was reviewed in the context of equation of state and observationsl results/ It was predicted that the maximum NS mass (MNS) exists in the range MNS ~ 2.2-2.9 M_Sun. However, recent observations of gravitationsl waves and other studies had suggested the higher mass limit of NSs, MNS ~ 3/2 M_Sun. The NS mass up to the value of MNS ~ 2 M_Sun is well understood, and with such a mass value it was meaning ful to discuss the "mass gap" ("m-gap") between the NS and black hole (BH) collapsars.The "m-gap" exists in between the highest mass of NS and the lowest mass of BH collapsars (Mm-gap ~ 2-5 M_Sun). in the mass distribution, the maximim population of NSs and BHs is located at MNS = 1.4 M_Sun and MBH = 6.7 M_Sun, respectively. However, recent ofservational results predicted filling the "m-gap" by the compact objects. In this paper, the concept of gravidynamics was reported to resolve the problem of peak likelihood value of gravitational mass at Mpeak = 6.7 M_Sun and the "m-gap" (Mm-gap ~ 2-5 M_Sun). This concept was based on a non-metric scalar-tensor model of gravitational interaction with localizable field energy. The gravidynamics model shows the total mass (MQ) of a compact relativistic object filled with matter of quark-gluon plasma of the radius r* = GMQ/c2 ~ 10 km, consistent with the "m-gap". It was conceptualized that the total measurable gravitational mass of such an extremely dense object consists of both matter and field, which is described by scalar-tensor components. This model is also useful for predicting the collapsars within the "m-gap".
