Existing theoretical literature suggests that defect-free, pristine carbon nanotubes (CNTs) interact weakly with many gas molecules like H 2 O, CO, NH 3 , H 2 , and so on. The case of NH 3 is particularly intriguing because this is in disagreement with experimentally observed changes in electrical conductance of CNTs upon exposure to these gases. In order to explain such discrepancy, we have carried out Density Functional Theory (DFT) investigations of the role of common atomistic defects in CNT (Stone-Wales, monovacancy, and interstitial) on the chemisorption of NH 3 . Computed binding energies, charge transfer, dissociation barriers, and vibrational modes are compared with existing experimental results on electrical conductance, thermal desorption and infrared spectroscopy. PACS: 61.46.+w, 85.35 [2,[9][10][11]. This is in disagreement not only with the observed drop in electrical conductance at room temperature, but also with recent temperature-programmed-desorption (TPD) measurements [12], which shows that most of the gas desorbs only at elevated temperatures (500-700 K).A logical resolution to the above problem would be to note that SWNTs are likely to have some defects incorporated either thermally or during high-temperature growth conditions. Also, they are not in isolation, and surrounding environment (oxygen, water vapor), or the substrate, or metal contacts at the ends might directly or indirectly provide a mechanism of binding of the gas molecules. Limited 2 investigations have been made on the effect of metal contacts, especially in connection with O 2 adsorption [13,14]. However, NH 3 adsorption appears to occur along the whole length of the tube [1], which suggests either topological defects on the tube itself, or an indirect mechanism due to involvement of solvents or the substrate.In this Letter, we investigate the role of three types of topological defects commonly considered for SWNTs and graphene sheet, i.e., a Stone-Wales (SW) defect [15] (i.e. a 5775 defect formed by bondrotation), a monovacancy (i.e. missing a C-atom), and an insterstitial (i.e. an extra bridging C). The presence of such geometric defects has recently been confirmed experimentally [16]. As a concrete model of s-SWNT, we chose the (8, 0) SWNT. All the defect and chemisorbed structures were created by suitably modifying the original defect-free tube (Fig. 1a). In order to speed up our calculations the initial structures were minimized with the COMPASS forcefield [17], followed by further relaxation with the DFT code (Fig. 1d); (ii) SW2, a chiral Stone-Wales defect (Fig. 1f); (iii) a monovacancy (V) (Fig. 1b); and (iv) an interstitial (I) (Fig. 1c). It also considers the situation in which an O 2 molecule has dissociated over a SW1 (Fig. 1e) [24]. Table 1 lists the respective DMol 3 -computed formation energies of these defects for supercells of two sizes, i.e., two and four times the smallest periodic segment of the (8, Table 1, we note that SW1 is energetically more stable than SW2, and is therefore the only SW d...