Spectral line width broadening in Rydberg gases, a phenomenon previously attributed to the many-body effect, was observed experimentally almost a decade ago. The observed line width was typically 80-100 times larger than the average interaction strength predicted from a binary interaction. The interpretation of such a phenomenon is usually based on the so-called diffusion model, where the line width broadening mostly originates from the diffusion of excitations. In this paper, we present a model calculation to show that diffusion is not the main mechanism to the line width broadening. We find that the rare pair fluctuation at small separation is the dominant factor contributing to this broadening. Our results give a width of about 20-30 times larger than the average interaction strength. More importantly, by turning off the diffusion process, we do not observe order of magnitude change in the spectral line width.PACS numbers: 32.80. Ee,34.20.Cf Rydberg gases have attracted renewed interest in recent years due to the unprecedented advancement in laser cooling and trapping [1,2,3,4,5,6,7,8,9]. Rydberg atoms, possessing a large dipole moment and long lifetime, can interact with each other coherently for relatively long times, which make it a potential candidate for quantum information processing [10,11]. There have been many experiments exploring the quantum manybody effects in Rydberg gases, e.g. spectral line broadening [1,2,3], number correlation [6,12,13] and collective excitation [8]. Many experimental results can be understood from the well-known dipole blockade effect: when two Rydberg atoms are close enough, the dipolar interaction will shift them out of resonance with the external driving laser, thus double excitation is greatly suppressed.In this paper, we are interested in the unusual line width broadening which was observed in experiments [1,2]. To be specific, we will consider the following two cases. (I), the main process is |np + |np ↔ |ns + |(n + 1)s for experiment [1], where the principal quantum number n is 23 and the maximal gas density is around 10 10 cm −3 . np, ns, and (n + 1)s are abbreviated as p, s, and s ′ , respectively. (II), the main process is |(n + 1)s + |n ′ s ↔ |np + |(n ′ + 1)p for experiment [2], where the principal quantum numbers n and n ′ are 24 and 33, respectively, and the maximal gas density is around 10 9 cm −3 for each of the s state. (n + 1)s, n ′ s, np, and (n ′ + 1)p are abbreviated as s, s ′ , p, and p ′ , respectively. For both cases, they express the creation process, e.g., in case (I), one atom makes a downward transition from the Rydberg state |p to |s , and the other atom makes an upward transition from |s ′ to |p , that is to say, creating ss ′ from a pp pair. The detuning between |pp and |ss ′ is controlled by a static electric field and the transition is allowed with dominant dipole moments µ ps and µ ps ′ . Here µ αβ denotes the transition dipole moment between states |α and |β . Similar notations will apply to case (II). In addition to the above creation p...