Roy, T.Mukherjee, G.Asgar, Md.A.Bhattacharyya, S.Bhattacharya, SoumikBhattacharya, C.Bhattacharya, S.Ghosh, T.K.Banerjee, K.Kundu, SamirRana, T.K.Roy, P.Pandey, R.Meena, J.Dhal, A.Palit, R.Saha, S.Sethi, J.Thakur, ShitalNaidu, B.S.Jadav, S.V.Dhonti, R.Pai, H.Goswami, A.2018-07-092018-07-090370-2693http://hdl.handle.net/1885/144952The High-spin states in 195 Tl, populated through the 185,187 Re( 13 C, xn) fusion evaporation reaction at the beam energy of 75 MeV, were studied using the Indian National Gamma Array (INGA). More than 50 new γ transitions have been placed in the proposed level scheme which is extended up to the excitation energy of ≈ 5.6 MeV and spin =22.5ħ . Two pairs of degenerate bands based on two different quasi-particle configurations have been identified in this nucleus indicating the first observation of such bands in an odd- A nucleus in A∼190 region and signify the first evidence of multiple chiral bands in a nucleus in this region. The total Routhian surface calculations predict triaxial shapes for both the configurations and thereby, support the experimental observation. The importance of multiple neutron holes in the i13/2 orbital and the stability of shapes for these two configurations have been discussed.Financial support of Department of Science & Technology, Govt. of India for clover detectors of INGA (Grant No. IR/S2/PF-03/2003-II) is greatfully acknowledged. One of the authors (S. Bhattacharya) acknowledges with thanks the financial support received as Raja Ramanna Fellowship from the Department of Atomic Energy, Govt. of India. T.R and Md. A.A acknowledge with thanks the financial support received as research fellows from the Department of Atomic Energy (DAE), Govt. of India.application/pdf© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3.http://creativecommons.org/licenses/by/3.0/Nuclear Structureγ -ray spectroscopyDoubly degenerate bandsTRS calculation2018-06-2710.1016/j.physletb.2018.06.0332018-07-01