In this study,we explore the potential of using TianQin missions to probe the local gravitational effects of dark matter.The TianQin project plans to launch satellites at both low and high orbits.High-precision orbit ...In this study,we explore the potential of using TianQin missions to probe the local gravitational effects of dark matter.The TianQin project plans to launch satellites at both low and high orbits.High-precision orbit determination is expected to aid in detecting Earth’s gravity or gravitational waves.By comparing the derived masses in low and high orbits,it is possible to constrain the amount of dark matter between the two spheres,hence placing a local constraint on dark matter’s gravitational effect.Our results show the capability of TianQin in detecting the density of dark matter around Earth,with an ultimate sensitivity to a value of 10^(-8) kg m^(-3).This detection limit surpasses the estimated bounds for the solar system and the observation results for our Galaxy by approximately 7 and 14 orders of magnitude,respectively.展开更多
基金Supported by the National Key Research and Development Program of China(2023YFC2206704)the National Key Research and Development Program of China(2020YFC2201400)+2 种基金the Natural Science Foundation of China(12173104)supported by the Guangdong Basic and Applied Basic Research Foundation(2023A1515111184)supported by the Natural Science Foundation of China(12373116).
文摘In this study,we explore the potential of using TianQin missions to probe the local gravitational effects of dark matter.The TianQin project plans to launch satellites at both low and high orbits.High-precision orbit determination is expected to aid in detecting Earth’s gravity or gravitational waves.By comparing the derived masses in low and high orbits,it is possible to constrain the amount of dark matter between the two spheres,hence placing a local constraint on dark matter’s gravitational effect.Our results show the capability of TianQin in detecting the density of dark matter around Earth,with an ultimate sensitivity to a value of 10^(-8) kg m^(-3).This detection limit surpasses the estimated bounds for the solar system and the observation results for our Galaxy by approximately 7 and 14 orders of magnitude,respectively.
