We construct an anomaly free supersymmetric U (1) ′ model with a secluded U (1) ′ -breaking sector. We study the one-loop effective potential at finite temperature, and show that there exists a strong enough first order electroweak phase transition for electroweak baryogenesis (EWBG) because of the large trilinear term A h hSH d Hu in the tree-level Higgs potential. Unlike in the MSSM, the lightest stop can be very heavy. We consider the non-local EWBG mechanism in the thin wall regime, and find that within uncertainties the observed baryon number can be generated from the τ lepton contribution, with the secluded sector playing an essential role. The chargino and neutralino contributions and the implications for the Z ′ mass and electric dipole moments are briefly discussed. PACS numbers: 12.60. Jv, 12.60.Cn [ UPR-1063-T ] The baryon asymmetry of the universe has been measured by WMAP [1]. Combining their data with other CMB and large scale structure results, they obtain the ratio of baryon density n B to entropy density sTo generate the baryon asymmetry, the Sakharov criteria [2] must be satisfied: (1) Baryon number (B) violation; (2) C and CP violation; (3) A departure from thermal equilibrium. Electroweak (EW) baryogenesis is especially interesting because the Sakharov criteria can be satisfied in the Standard Model (SM) [3]. However, in the SM the electroweak phase transition (EWPT) cannot be strongly first order for the experimentally allowed Higgs mass, and the CP violation from the CKM matrix is too small. In the Minimal Supersymmetric Standard Model (MSSM), although there are additional sources of CP violation in the supersymmetry breaking parameters, a strong enough first order EWPT requires that the lightest stop quark mass be smaller than the top quark mass ∼ 175 GeV. Also, the mass of the lightest CP even Higgs must be smaller than 120 GeV, which leaves a small window above the current limit [4]. In the Next to Minimal Supersymmetric Standard Model (NMSSM), a trilinear term A h hSH d H u in the tree-level Higgs potential may induce a strong enough first order EWPT [5,6], and the effective µ parameter is given by h S from the Yukawa term hSH d H u in the superpotential in the best-motivated versions. However, most versions either involve a discrete symmetry and serious cosmological domain wall problems [7], or reintroduce the µ problem [6].The possibility of an extra U (1) ′ gauge symmetry is well-motivated in superstring constructions [8]. Similar to the NMSSM, an extra U (1) ′ can provide an elegant solution to the µ problem due to the Yukawa term hSH d H u [9,10]. However, there are no discrete symmetries or domain wall problems. The MSSM upper bound of M Z on the tree-level mass of the lightest MSSM Higgs scalar is relaxed, both in models with a U (1) ′ and in the NMSSM, because of the Yukawa term hSH d H u and the U (1) ′ D-term [11]. Higgs masses lighter than those allowed by LEP in the MSSM are also possible, with the limits relaxed by mixings between Higgs doublets and singlets. There are ...