Fig. 3: Ground state orbital entanglement diagrams (from MPS(24e,24o) calculations with 12 occupied and 12 virtual orbitals) for the [OUO]+2 ion, CUO, and \({({{{{{{{{\rm{R}}}}}}}}}^{{{{{{{{\rm{a}}}}}}}}})}_{3}{{{{{{{{\rm{NU}}}}}}}}}^{{{{{{{{\rm{VI}}}}}}}}}{{{{{{{\rm{N}}}}}}}}\). | Nature Communications

Fig. 3: Ground state orbital entanglement diagrams (from MPS(24e,24o) calculations with 12 occupied and 12 virtual orbitals) for the [OUO]+2 ion, CUO, and \({({{{{{{{{\rm{R}}}}}}}}}^{{{{{{{{\rm{a}}}}}}}}})}_{3}{{{{{{{{\rm{NU}}}}}}}}}^{{{{{{{{\rm{VI}}}}}}}}}{{{{{{{\rm{N}}}}}}}}\).

From: Actinide inverse trans influence versus cooperative pushing from below and multi-center bonding

Fig. 3: Ground state orbital entanglement diagrams (from MPS(24e,24o) calculations with 12 occupied and 12 virtual orbitals) for the [OUO]+2 ion, CUO, and 
                        
                          
                        
                        $${({{{{{{{{\rm{R}}}}}}}}}^{{{{{{{{\rm{a}}}}}}}}})}_{3}{{{{{{{{\rm{NU}}}}}}}}}^{{{{{{{{\rm{VI}}}}}}}}}{{{{{{{\rm{N}}}}}}}}$$
                        
                          
                            
                              
                                (
                                
                                  
                                    
                                      R
                                    
                                    
                                      a
                                    
                                  
                                
                                )
                              
                            
                            
                              3
                            
                          
                          
                            
                              NU
                            
                            
                              VI
                            
                          
                          N
                        
                      .

Orbitals involving the rearward 2sp hybrid are highlighted by a red dashed line. MPS natural occupation numbers are given in black for the entangled orbitals. The area of the red circles is proportional to an orbital’s single-orbital entropy, while the thickness of connecting lines is proportional to the mutual orbital pair information. Orbital isosurface values are ±0.04 atomic units and rendered in red/blue vs. orange/yellow for high- vs. low-occupancy orbitals, respectively.

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