论文标题
限制了Yukawa抑制牛顿的潜力，即星球的iNpop19a
Constraint on the Yukawa suppression of the Newtonian potential from the planetary ephemeris INPOP19a
论文作者
论文摘要
为了改善我们对Yukawa抑制牛顿电位的抑制，我们使用埃菲默里人INPOP（19a）的最新解决方案，这通常与重力的质量相关。与Ephemeris Inpop17a不同，发现几个残差在康普顿波长$λ_g$的幅度大致相同的幅度下显着降解。结果，我们引入了一个新颖的统计标准，以通过INPOP19A得出约束。在检查它在InPOP17B上应用时与我们先前的结果一致的约束后，我们将方法应用于新解决方案INPOP19A。 We show that the residuals of Mars orbiters, Cassini, Messenger, and Juno, degrade significantly when $λ_g \leq$ $3.43 \times 10^{13}$ km with a 99,7% confidence level -- corresponding to a graviton mass bigger than $3.62 \times 10^{-23}$ eV$/c^2$.这是对康普顿波长的严格限制，比从辐射方案中的Ligo-Virgo协作中从第一个重力波瞬态目录获得的康普顿波长限制，因为我们的90％C.L.限制读取$λ_g> 3.93 \ times 10^{13} $ km（$ m_g <3.16 \ times 10^{ - 23} $ ev $/c^2 $）。
We use the latest solution of the ephemeris INPOP (19a) in order to improve our previous constraint on the existence of a Yukawa suppression to the Newtonian potential, generically associated to a graviton's mass. Unlike the ephemeris INPOP17a, several residuals are found to degrade significantly at roughly the same amplitudes of the Compton wavelength $λ_g$. As a consequence, we introduce a novel statistical criterion in order to derive the constraint with INPOP19a. After checking that it leads to a constraint consistent with our previous result when applied on INPOP17b, we apply the method to the new solution INPOP19a. We show that the residuals of Mars orbiters, Cassini, Messenger, and Juno, degrade significantly when $λ_g \leq$ $3.43 \times 10^{13}$ km with a 99,7% confidence level -- corresponding to a graviton mass bigger than $3.62 \times 10^{-23}$ eV$/c^2$. This is a stronger constraint on the Compton wavelength than the one obtained from the first gravitational-wave transient catalog by the LIGO-Virgo collaboration in the radiative regime, since our 90% C.L. limit reads $λ_g >3.93 \times 10^{13}$ km ($m_g <3.16 \times 10^{-23}$ eV$/c^2$).
