Table 3.

The mass spectra (in GeV) for the supersymmetric sector and the relic density ${\Omega }_{\mathit{DM}}{h}^2$ values of the benchmark points given in Table 2 for the Secluded $U{(1)}^{\prime }$

$\mathrm{M}asses$	$\mathrm{B}P1$	$\mathrm{B}P2$	$\mathrm{B}P3$	Bounds
$m_{Z^{\prime }}$	4250	4069	5195	3900 [76]
$m_{H_i^0,i=1,\dots ,6}$	(125.9, 543, 671, 1077, 4237, 17719)	(125.0, 557, 1148, 2418, 4171, 19151)	(125.3, 524, 1045, 1611, 5210, 22171)	$m_{H_1^0}=125.2$ [76]
$m_{A_i^0,i=1,\dots ,4}$	(550, 719, 1012, 17718)	(563, 592, 20769, 19151)	(531, 572, 1882, 22170)	$m_{A_1^0}>93.4$ [76]
$m_{{\tilde{\chi }}_i^0,i=1,\dots ,5}$	(51, 167, 262, 312, 613)	(48, 269, 328, 762, 763)	(52, 195, 264, 303, 360)	$m_{{\tilde{\chi }}_1^0}>50$ [76]
$m_{{\tilde{\chi }}_i^0,i=6,\dots ,9}$	(1226, 2004, 4222, 4638)	(1170, 1740, 4047, 4237)	(1036, 1939, 4908, 5551)	–
$(m_{{\tilde{\chi }}_1^{\pm }},m_{{\tilde{\chi }}_2^{\pm }})$	(256, 2004)	(267, 763)	(192, 359)	$m_{{\tilde{\chi }}_1^{\pm }}>103.5$ [76]
$m_{H^{\pm }}$	540.9	554.9	522.4	$m_{H^{\pm }}>80$ [76]
$(m_{{\tilde{e}}_L},m_{{\tilde{\mu }}_L},m_{{\tilde{\tau }}_1})$	(503, 503, 457)	503	(1412, 1412, 473)	$m_{\tilde{\ell }}>(82-107)$ [76]
$(m_{{\tilde{e}}_R},m_{{\tilde{\mu }}_R},m_{{\tilde{\tau }}_2})$	(457, 457, 503)	1850	(473, 473, 1412)	$m_{\tilde{\ell }}>(82-107)$ [76]
$(m_{{\tilde{\nu }}_e},m_{{\tilde{\nu }}_{\mu }},m_{{\tilde{\nu }}_{\tau }})$	501	501	1412	$m_{{\tilde{\nu }}_{\ell }}>41$ [76]
$(m_{{\tilde{\nu }}_{\mathit{eR}}},m_{{\tilde{\nu }}_{\mu R}},m_{{\tilde{\nu }}_{\tau R}})$	553	3472	645	–
${\Omega }_{\mathit{DM}}{h}^2$	0.117	0.121	0.119	0.111 [75]