Effects of Newtonian gravitational self-interaction in
harmonically trapped quantum systems
Effects of Newtonian gravitational self-interaction in
harmonically trapped quantum systems
 
  The Schrödinger–Newton equation has gained attention in the recent past as a nonlinear modification of the Schrödinger equation due to a gravitational self-interaction. Such a modification is expected from a fundamentally semi-classical theory of gravity and can, therefore, be considered a test case for the necessity of the quantisation of the gravitational field. Here we provide a thorough study of the effects of the Schrödinger–Newton equation for a micron-sized sphere trapped in a harmonic oscillator potential. We discuss both the effect on the energy eigenstates and the dynamical behaviour of squeezed states, covering the experimentally relevant parameter regimes.
  
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      Grossardt, Andre
      
        b64b259c-ea5e-41bd-a20f-7df2a710b247
      
     
  
    
      Bateman, James
      
        05b8f150-3d00-49f6-bf35-3d535b773b53
      
     
  
    
      Ulbricht, Hendrik
      
        5060dd43-2dc1-47f8-9339-c1a26719527d
      
     
  
    
      Bassi, Angelo
      
        374a70f7-61f8-4656-bb45-5857695750f1
      
     
  
  
   
  
  
    
    
  
    
    
  
  
    
      Grossardt, Andre
      
        b64b259c-ea5e-41bd-a20f-7df2a710b247
      
     
  
    
      Bateman, James
      
        05b8f150-3d00-49f6-bf35-3d535b773b53
      
     
  
    
      Ulbricht, Hendrik
      
        5060dd43-2dc1-47f8-9339-c1a26719527d
      
     
  
    
      Bassi, Angelo
      
        374a70f7-61f8-4656-bb45-5857695750f1
      
     
  
       
    
 
  
    
      
  
  
  
  
  
  
    Grossardt, Andre, Bateman, James, Ulbricht, Hendrik and Bassi, Angelo
  
  
  
  
   
    (2016)
  
  
    
    Effects of Newtonian gravitational self-interaction in
harmonically trapped quantum systems.
  
  
  
  
    Scientific Reports, 6 (30840), .
  
   (doi:10.1038/srep30840). 
  
  
   
  
  
  
  
  
   
  
    
    
      
        
          Abstract
          The Schrödinger–Newton equation has gained attention in the recent past as a nonlinear modification of the Schrödinger equation due to a gravitational self-interaction. Such a modification is expected from a fundamentally semi-classical theory of gravity and can, therefore, be considered a test case for the necessity of the quantisation of the gravitational field. Here we provide a thorough study of the effects of the Schrödinger–Newton equation for a micron-sized sphere trapped in a harmonic oscillator potential. We discuss both the effect on the energy eigenstates and the dynamical behaviour of squeezed states, covering the experimentally relevant parameter regimes.
         
      
      
        
          
            
  
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 srep30840.pdf
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  More information
  
    
      Accepted/In Press date: 7 July 2016
 
    
      e-pub ahead of print date: 4 August 2016
 
    
  
  
    
  
    
  
    
  
    
  
    
  
    
  
    
     
        Organisations:
        Quantum, Light & Matter Group
      
    
  
    
  
  
  
    
  
  
        Identifiers
        Local EPrints ID: 402020
        URI: http://eprints.soton.ac.uk/id/eprint/402020
        
          
        
        
        
        
          PURE UUID: 5bbde764-2c9f-4e83-b4cc-479c110a6815
        
  
    
        
          
        
    
        
          
        
    
        
          
            
              
            
          
        
    
        
          
        
    
  
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  Date deposited: 26 Oct 2016 14:04
  Last modified: 21 Aug 2025 02:02
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      Contributors
      
          
          Author:
          
            
            
              Andre Grossardt
            
          
        
      
          
          Author:
          
            
            
              James Bateman
            
          
        
      
        
      
          
          Author:
          
            
            
              Angelo Bassi
            
          
        
      
      
      
    
  
   
  
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