shows the difference between observed (black) and calculated patterns (red). Vertical ticks indicate

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Intensity (arb. unit) a 5 K No disorder Mn-Pt disorder 5 K Mn-Ga disorder 5 K b 5 K Observed Calculated Difference Bragg positions 24 28 32 2 4 6 8 2 4 2θ (degree) 2θ (degree) Supplementary Figure. Powder neutron diffraction on Pt 2 MnGa at 5 K. The green curve shows the difference between observed (black) and calculated patterns (red). Vertical ticks indicate the nuclear Bragg peak positions. a The (2) and () Bragg peaks (black circles) have been fitted (red solid lines) by assuming (i) no disorder, (ii) Mn(2a)/Pt(4d) disorder, and (iii) Mn(2a)/Ga(2b) disorder. b Comparison of neutron diffraction patterns for the whole angular range.

specific heat C V [k B / atom] M / M s exchange coupling, J ij [mev] 4 2-2 AFM.5 2 2.5 3 3.5 4 distance, R/a.8.6 R/a = 2. R/a = 2.6.8.6.4 R/a = 2.87 (a) (b).4.2.2 2 3 4 5 T [K] 2 3 4 5 T [K] Supplementary Figure 2. a Isotropic exchange coupling constants J ij computed as functions of distance R (in the units of a) between i and j sites within Mn(2a) sublattice. b Monte-Carlo simulated M/M S temperature dependencies of the Heisenberg model parametrized by the computed J ij. Solid line corresponds to the minimal cluster size needed to set the AFM order, dashed - by one shall smaller cluster. The inset shows the temperature dependency of the specific heat C V (computed for the largest technically possible cluster size of R/a = 2.87) which indicates the position of T N by the local maximum. 2

Supplementary Note Crystal structure from neutron diffraction Supplementary Figure shows the observed and calculated neutron diffraction patterns at 5 K (paramagnetic phase) in the range of 2 < 2θ < 4. All peaks are well indexed in Rietveld refinement assuming the space groupi4/mmm as in case of the X-ray diffraction. Refined lattice parameters are a = b = 4.3 Å, c = 7.24 Å. In a perfectly ordered unit cell, Mn, Ga and Pt atoms would occupy 2a(,,), 2b(,,.5) and 4d(,.5,.25) Wyckoff positions, respectively. On the other hand, our Rietveld fit indicates possible presence of Mn(2a)-Ga(2b) disorder: by comparing several reasonable chemical configurations (focusing on (2) and () Bragg peaks), the perfect agreement is provided by assuming 33 % of Mn(2a)-Ga(2b) disorder (lower panel in Supplementary Figure a). Supplementary Note 2 Monte-Carlo simulations Here we try to figure which mechanisms are responsible for setting such a long range ground-state modulation (by assuming a perfectly ordered structure). Since the relativistic effects do not affect the ground-state q vector substantially, in the following we calculate the isotropic exchange coupling constantsj ij using the real-space approach implemented in the SPR-KKR Green s function method. 2 In Supplementary Figure 2 a they are plotted as functions of distance between the interacting sites i and j. Here, we drop all interactions involving Pt and Ga atoms as insignificant, 3

by leaving only those between Mn atoms. It follows, that all nearest Mn(2a)-Mn(2a) interactions are parallel (J > ), whereas the antiparallel ones (J < ) are encountered by starting from R/a = 2 (6-th shell within (2a)-sublattice). As it is shown by M(T)/M S curves (Supplementary Figure 2 b) obtained by the Monte-Carlo simulation (ALPS package 3 ) of the classical Heisenberg model (H = i>j J ije i e j, wheree i,j are the unity vectors along the local magnetization directions on i and j sites), the AFM order sets in by including all interactions at least up to R/a 2.6 (7-th shell); accounting of the higher shells does not affect the M(T) behavior anymore. Such a superposition of the strong nearest parallel and the weaker long-range antiparallel exchange interactions typically allows for the long-range spin-spiral order. Its direction (q []) follows from the symmetry reasons: the 7-th shell, critical for setting up the AFM order, contains 8 atoms at R = (±a,,±c) and (,±a,±c), situated above and below the ab-plane of the central atom. The corresponding Neel temperature can be estimated from the peak of the magnetic specific heatc V (T) computed for the largest cluster size (T N 35 K atr/a 2.87, see the inset in Supplementary Figure 2 b). This again reasonably agrees with experimentalm(t) slope change. Supplementary References. Liechtenstein, A. I., Katsnelson, M. I., Antropov, V. P. & Gubanov, V. A. Local spin density functional approach to the theory of exchange interactions in ferromagnetic metals and alloys. J. Magn. Magn. Materials 67, 65 74 (987). 2. Ebert, H., Ködderitzsch, D. & Minár, J. Calculating condensed matter properties using the KKR-Green s function method - recent developments and applications. Rep. Prog. Phys. 74, 965 (2). 4

3. Bauer, B. et al. The ALPS project release 2.: open source software for strongly correlated systems. J. Stat. Mech.: Theory and Experiment 2, P5 (2). 5