The single-mode Dicke model is well known to undergo a quantum phase transition from the so-called normal phase to the superradiant phase (hereinafter called the 'superradiant quantum phase transition'). Normally, quantum phase transitions can be identified by the critical behavior of quantities such as entanglement, quantum fluctuations, and fidelity. In this paper, we study the role of the quantum Fisher information (QFI) of both the field mode and the atoms in the ground state of the Dicke Hamiltonian. For a finite but large number of atoms, our numerical results show that near the critical atom-field coupling, the QFI of the atomic and the field subsystems can surpass their classical limits, due to the appearance of nonclassical quadrature squeezing. As the coupling increases far beyond the critical point, each subsystem becomes a highly mixed state, which degrades the QFI and hence the ultimate phase sensitivity. In the thermodynamic limit, we present the analytical results of the QFI and their relationship with the reduced variances of the field mode and the atoms. For each subsystem, we find that there is a singularity in the derivative of the QFI at the critical point, a clear signature of the quantum criticality in the Dicke model.Quantum phase transitions in many-body systems are of fundamental interest [1] and have potential applications in quantum information [2][3][4][5][6][7] and quantum metrology [8][9][10][11][12][13][14][15]. Consider, for instance, a collection of N two-level atoms interacting with a single-mode bosonic field, described by the Dicke model (with = 1) [16]:z 0 whereb andˆ † b are annihilation and creation operators of the bosonic field with oscillation frequency ω, which is nearly resonant with the atomic energy splitting ω 0 . The collective spin operators σ ≡ˆ±ˆ= ∑± ± J J iJ x y k k and σ = ∑Ĵ 2 z k k z obey the SU(2) Lie algebra, where σ ± k and σ k z are Pauli operators of the kth atom. The atom-field coupling strength λ ∝ N V depends on the atomic density N V . For a finite number of atoms N (= j 2 ), the Hamiltonian (1) commutes with the parity, where Tr A (Tr B ) is the partial trace of the ground state |g over the atomic (bosonic field) degrees of freedom. The QFI is one of the central quantities used to qualify the utility of an input state [35,36], especially in Mach-Zehnder (or, equivalently, Ramsey) interferometer-based phase or parameter estimation. The achievable phase sensitivity is well known to be limited by the quantum Cramér-Rao bound δφ ρ ∝ˆF G 1 ( , ) min in , where the QFI ρF G ( , ) in depends on the input state ρ in and the New J. Phys. 16 (2014) 063039 T-L Wang et al B 2 . Therefore, the ultimate sensitivity is limited by δφ =n 1/(2 ) min cl , known as New J. Phys. 16 (2014) 063039 T-L Wang et al