  The proposal of pilgrim dark energy is based on speculation that phantom-like
dark energy (with strong enough resistive force) can prevent black hole
formation in the universe. We explore this phenomenon in loop quantum cosmology
framework by taking Hubble horizon as an infra-red cutoff in pilgrim dark
energy. We evaluate the cosmological parameters such as Hubble, equation of
state parameter, squared speed of sound and also cosmological planes like
$\omega_{\vartheta}-\omega'_{\vartheta}$ and $r-s$ on the basis of pilgrim dark
energy parameter ($u$) and interacting parameter ($d^2$). It is found that
values of Hubble parameter lies in the range $74^{+0.005}_{-0.005}$. It is
mentioned here that equation state parameter lies within the ranges
$-1\mp0.00005$ for $u=2, 1$ and $(-1.12,-1), (-5,-1)$ for $u=-1,-2$,
respectively. Also, $\omega_{\vartheta}-\omega'_{\vartheta}$ planes provide
$\Lambda$CDM limit, freezing and thawing regions for all cases of $u$. It is
also interesting to mention here that $\omega_{\vartheta}-\omega'_{\vartheta}$
planes lie in the range ($\omega_{\vartheta}=-1.13^{+0.24}_{-0.25},
\omega'_{\vartheta}<1.32$). In addition, $r-s$ planes also corresponds to
$\Lambda$CDM for all cases of $u$. Finally, it is remarked that all the above
constraints of cosmological parameters shows consistency with different
observational data like Planck, WP, BAO, $H_0$ and SNLS.
