  To solve the fine-tuning problem in $\mu$-Term Hybrid Inflation, we will
realize the supersymmetry scenario with the TeV-scale supersymmetric particles
and intermediate-scale gravitino from anomaly mediation, which can be
consistent with the WMAP and Planck experiments. Moreover, we for the first
time propose the $\mu$-term hybrid inflation in no-scale supergravity. With
four Scenarios for the $SU(3)_C\times SU(2)_L\times SU(2)_R\times U(1)_{B-L}$
model, we show that the correct scalar spectral index $n_s$ can be obtained,
while the tensor-to-scalar ratio $r$ is prediced to be tiny, about
$10^{-10}-10^{-8}$. Also, the $SU(2)_R\times U(1)_{B-L}$ symmetry breaking
scale is around $10^{14}$ GeV, and all the supersymmetric particles except
gravitino are around TeV scale while gravitino mass is around $10^{9-10}$ GeV.
Considering the complete potential terms linear in $S$, we for the first time
show that the tadpole term, which is the key for such kind of inflationary
models to be consistent with the observed scalar spectral index, vanishes after
inflation. Thus, to obtain the $\mu$ term, we need to generate the
supersymmetry breaking soft term $A^{S \Phi \Phi'}_{\kappa} \kappa S \Phi
\Phi'$ due to $A^{S \Phi \Phi'}_{\kappa}=0 $ in no-scale supergravity, where
$\Phi$ and $\Phi'$ are vector-like Higgs fields at high energy. We show that
the proper $A^{S \Phi \Phi'}_{\kappa} \kappa S \Phi \Phi'$ term can be obtained
in the M-theory inspired no-scale supergravity. We also point out that $A^{S
\Phi \Phi'}_{\kappa}$ around 700 GeV can be generated via the renormalization
group equation running from string scale.
