Overview of Fundamental Physics and Cosmology with TianQin
The paper "Fundamental Physics and Cosmology with TianQin" explores the prospective capabilities of the TianQin mission in advancing our understanding of both fundamental physics and cosmology. TianQin is a planned space-based gravitational wave (GW) detector that aims to detect GWs primarily in the millihertz frequency range (10−4∼1 Hz). The mission's scientific objectives cover a broad spectrum, promising significant contributions to gravitational physics and cosmological research.
Key Scientific Potential of TianQin
Gravitational Physics
- Testing General Relativity (GR): TianQin will provide a unique opportunity to test the predictions of GR in the strong-field regime. By observing the dynamics of massive black hole binaries (MBHBs) and extreme mass-ratio inspirals (EMRIs), TianQin can test the validity of GR and probe for potential deviations. The mission could detect higher-order and non-linear gravitational wave (GW) modes, thereby enhancing our understanding of the non-linearity of Einstein's equations.
- Detection of Novel Gravitational Effects: The mission is equipped to search for GW memory effects and explore the Kerr nature of astrophysical black holes. The memory effect, a non-linear feature predicted by GR, remains elusive and its detection would reaffirm our understanding of gravitational phenomena. Moreover, by examining Kerr black holes, TianQin could test hypotheses about black holes, which predict their complete characterization by mass and spin alone.
- Exploration of Modified Gravity Theories: TianQin will investigate various modified theories of gravity (MGTs) that predict deviations from GR in terms of GW polarizations, dispersion relations, and generation mechanisms. This involves testing theories like Einstein-Aether and Chern-Simons gravity, which introduce additional gravitational interactions or modify existing ones.
Cosmological Insights
TianQin extends its research focus to cosmic phenomena and the universe's large-scale structure:
- Dark Energy and Expansion History: Utilizing GW standard sirens like MBHBs, TianQin will allow scientists to measure the cosmos's expansion rate across vast time scales. This can improve constraints on the Hubble constant and offer insights into the dark energy equation of state, addressing unsolved issues like the Hubble tension—a discrepancy in the measured expansion rate of the universe.
- Primordial Universe and Dark Matter: The mission has the capacity to detect stochastic GW backgrounds generated by phenomena such as cosmic strings and phase transitions in the early universe. These observations could provide clues about new particles and interactions beyond the Standard Model of Particle Physics, including potential dark matter candidates.
- Primordial Black Holes (PBHs): TianQin will explore the existence of PBHs, which could account for some fraction of dark matter and offer a unique probe into the conditions of the early universe when density fluctuations may have led to their formation.
Implications and Future Directions
The paper outlines the role of TianQin in potentially transforming our understanding of fundamental physics and cosmology. By exploring new frontiers in gravitational physics and providing alternative methods for cosmological studies, TianQin could address longstanding issues such as the quantum nature of gravity and the expansion history of the universe. The synergy with upcoming GW detectors, like LISA and third-generation ground-based observatories, will enhance its scientific yield by enabling joint observations and data integration across different frequency bands.
TianQin is set to commence a new age of precision tests in the millihertz GW frequency range. It marks a pivotal step toward unraveling complex physics, offering a window into the universe's most enigmatic phenomena. The mission will likely stimulate further theoretical developments and shape the trajectory of research in cosmology and gravitational physics, providing a basis for breakthroughs in these fields.