由气泡产生的右手中微子引发的宇宙对撞机引力波:检验跷跷板、轻子生成和暗物质
Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
AI总结:
本文研究最小I型跷跷板框架中,由单态标量驱动的一阶相变通过气泡碰撞产生右手中微子,从而产生新型低频引力波,并探讨其用于检验轻子生成和暗物质的可能性。
摘要:
我们研究了一个最小I型跷跷板框架,其中由单态标量驱动的一阶相变(FOPT)通过气泡碰撞产生右手中微子(RHN),实现了一个探测超高能标尺度的宇宙级对撞机。由此产生的RHN分布除了标准气泡碰撞贡献外,还产生了新型低频引力波(GW)。稳定的最轻RHN可以解释观测到的暗物质(DM)遗迹丰度,其质量低至$M_{1} \equiv m_{\rm DM} \gtrsim 10^{6}\,\mathrm{GeV}$,相应的新型GW信号可在LISA、ET和即将到来的LVK探测器中观测到。如果RHN不稳定,其CP破坏衰变通过轻子生成产生观测到的重子不对称性,要求$M_{1} \gtrsim 10^{11}\,\mathrm{GeV}$和相变温度$T_* \gtrsim 10^{6}\,\mathrm{GeV}$,此时新型GW谱可在ET、BBO和即将到来的LVK中探测到。如果RHN衰变还填充了质量$m_\chi \in [10^{-4},10^{4}],\mathrm{GeV}$的暗区费米子,则对于$T_* \gtrsim 10^{7}\,\mathrm{GeV}$和$M_{1} \gtrsim 10^{9}\,\mathrm{GeV}$,可实现重子和不对称暗物质的共同起源,自然解释$\Omega_{\rm DM} \simeq 5\Omega_{\rm B}$。相应的GW信号可通过LISA、ET和BBO检验。最后,我们分析了一个基于全局$U(1)_N \times U(1)_{\rm B-L}$扩展的UV完备多Majoron模型,该模型由轻子质量层级启发,我们称之为Mojaron对撞机。该模型中的相应FOPT在$U(1)_N$对称性破缺期间由RHN产生留下了独特的GW特征,可被BBO、ET和即将到来的LVK探测。成功的轻子生成要求最重RHN质量$M_3 \sim 10^{10}\,\mathrm{GeV}$和$U(1)_N$破缺vev $v_2 \sim \mathcal{O}(\mathrm{TeV})$,后者设定了跷跷板标度。
英文摘要:
We study a minimal type-I seesaw framework in which a first-order phase transition (FOPT), driven by a singlet scalar, produces right-handed neutrinos (RHNs) through bubble collisions, realizing a cosmic-scale collider that probes ultra-high energy scales. The resulting RHN distribution sources novel low-frequency gravitational-waves (GWs) in addition to the standard bubble-collision contribution. A stable lightest RHN can account for the observed dark matter (DM) relic abundance for masses as low as $M_{1} \equiv m_{\rm DM} \gtrsim 10^{6}\,\mathrm{GeV}$, with the associated novel GW signal accessible in LISA, ET and upcoming LVK detectors. If the RHNs are unstable, their CP-violating decays generate the observed baryon asymmetry via leptogenesis for $M_{1} \gtrsim 10^{11}\,\mathrm{GeV}$ and phase transition temperatures $T_* \gtrsim 10^{6}\,\mathrm{GeV}$, for which the novel GW spectrum is detectable in ET, BBO and upcoming LVK. If RHN decays also populate a dark-sector fermion with mass $m_χ \in [10^{-4},10^{4}],\mathrm{GeV}$, successful co-genesis of baryons and asymmetric dark matter occurs for $T_* \gtrsim 10^{7}\,\mathrm{GeV}$ and $M_{1} \gtrsim 10^{9}\,\mathrm{GeV}$, naturally explaining $Ω_{\rm DM} \simeq 5Ω_{\rm B}$. The corresponding GW signals are testable with LISA, ET, and BBO. Finally, we analyze a UV-complete multi-Majoron model, based on a global $U(1)_N \times U(1)_{\rm B-L}$ extension, motivated from the hierarchy of lepton masses, which we dub as Mojaron collider. The corresponding FOPT in this model leaves a distinctive GW signature arising from RHN production during $U(1)_N$ symmetry breaking detectable by BBO, ET and upcoming LVK. Successful leptogenesis is realized for heaviest RHN mass $M_3 \sim 10^{10}\,\mathrm{GeV}$ and a $U(1)_N$ breaking vev $v_2 \sim \mathcal{O}(\mathrm{TeV})$, which sets the seesaw scale.
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