scholarly journals A Theoretical Stereoselectivity Model of Photochemical Denitrogenations of Diazoalkanes Towards Strained 1,3-Dihalogenated Bicyclobutanes

Author(s):  
Jingbai Li ◽  
Rachel Stein ◽  
Steven Lopez

<p>Photochemical reactions exemplify ‘green’ chemistry and are essential for synthesizing highly strained molecules with mild conditions with light. The light-promoted denitrogenation of bicyclic azoalkanes affords functionalized, stereoenriched bicyclo[1.1.0]butanes. We revisited these reactions with multireference calculations and non-adiabatic molecular dynamics (NAMD) simulations for a series of diazabicyclo[2.1.1]hexenes to predict the photophysics, reactivities, and stereoselectivities. We used complete active space self-consistent field (CASSCF) calculations with an (8,8) active space and ANO-S-VDZP basis set; the CASSCF energies were corrected with CASPT2(8,8)/ANO-S-VDZP. The excitation is consistently n→π* and ranges from 3.77–3.91 eV for the diazabicyclo[2.1.1]hexenes. Minimum energy path calculations showed stepwise C–N bond breaking and led to a minimum energy crossing point, which favors the stereochemical ‘double inversion’ bicyclobutane product. Wigner sampling of <b>1</b> provided Franck-Condon points for 692 NAMD trajectories. We identified competing complete stereoselective and stereochemical scrambling pathways. The stereoselective pathways feature concerted bicyclobutane inversion and N<sub>2</sub> extrusion. The stereochemical scrambling pathways involve N<sub>2</sub> extrusion followed by bicyclobutane planarization, leading to non-stereoselective outcomes. The predicted diastereomeric excess almost exactly match experiment (calc<i>.d.e.</i>=46% <i>vs.</i> exp<i>.d.e.</i>=47%). Our NAMD simulations with 672, 568, and 596 trajectories for <b>1-F</b>, <b>1-Cl</b>, and <b>1-Br</b> predicted diastereomeric excess (<i>d.e.</i>) of 94–97% for the double inversion products. Halogenation significantly perturbs the potential energy surface (PES) towards the retention products because of powerful hyperconjugative interactions. The n<sub>C</sub>→σ<sup>*</sup><sub>C–X</sub>,<sub> </sub>X = F, Cl, Br hyperconjugative interaction leads to a broadened shoulder region on the PES for double inversion.</p>

2020 ◽  
Author(s):  
Jingbai Li ◽  
Rachel Stein ◽  
Steven Lopez

<p>Photochemical reactions exemplify ‘green’ chemistry and are essential for synthesizing highly strained molecules with mild conditions with light. The light-promoted denitrogenation of bicyclic azoalkanes affords functionalized, stereoenriched bicyclo[1.1.0]butanes. We revisited these reactions with multireference calculations and non-adiabatic molecular dynamics (NAMD) simulations for a series of diazabicyclo[2.1.1]hexenes to predict the photophysics, reactivities, and stereoselectivities. We used complete active space self-consistent field (CASSCF) calculations with an (8,8) active space and ANO-S-VDZP basis set; the CASSCF energies were corrected with CASPT2(8,8)/ANO-S-VDZP. The excitation is consistently n→π* and ranges from 3.77–3.91 eV for the diazabicyclo[2.1.1]hexenes. Minimum energy path calculations showed stepwise C–N bond breaking and led to a minimum energy crossing point, which favors the stereochemical ‘double inversion’ bicyclobutane product. Wigner sampling of <b>1</b> provided Franck-Condon points for 692 NAMD trajectories. We identified competing complete stereoselective and stereochemical scrambling pathways. The stereoselective pathways feature concerted bicyclobutane inversion and N<sub>2</sub> extrusion. The stereochemical scrambling pathways involve N<sub>2</sub> extrusion followed by bicyclobutane planarization, leading to non-stereoselective outcomes. The predicted diastereomeric excess almost exactly match experiment (calc<i>.d.e.</i>=46% <i>vs.</i> exp<i>.d.e.</i>=47%). Our NAMD simulations with 672, 568, and 596 trajectories for <b>1-F</b>, <b>1-Cl</b>, and <b>1-Br</b> predicted diastereomeric excess (<i>d.e.</i>) of 94–97% for the double inversion products. Halogenation significantly perturbs the potential energy surface (PES) towards the retention products because of powerful hyperconjugative interactions. The n<sub>C</sub>→σ<sup>*</sup><sub>C–X</sub>,<sub> </sub>X = F, Cl, Br hyperconjugative interaction leads to a broadened shoulder region on the PES for double inversion.</p>


2020 ◽  
Author(s):  
Jingbai Li ◽  
Steven Lopez

<p>Sunlight is a renewable energy source that can be stored in chemical bonds using photochemical reactions. The synthesis of exotic and strained molecules is especially attractive with photochemical techniques because of the associated efficient and mild reaction conditions. We have used complete active space self-consistent field (CASSCF) calculations with an (8,7) active space and the ANO-S-VDZP basis set to understand the photophysics and subsequent photochemistry of a possible cubane precursor tricyclo[4,2,0,0<sup>2,5</sup>]octa-3,7-diene (<b>1</b>). The energies were corrected with a second-order perturbative correction CASPT2(8,7)/ANO-S-VDZP. The S<sub>0</sub>→S<sub>1</sub> vertical excitation energy of <b>1</b> is 6.25 eV, whose nature is π→π<sup>*</sup> excitation. The minimum energy path from the S<sub>1</sub> Franck-Condon point leads directly to a 4π-disrotatory electrocyclic ring-opening reaction to afford bicyclo[4,2,0]octa-2,4,7-triene. The 2D potential energy surface scan located a rhomboidal S<sub>1</sub>/S<sub>0</sub> minimum energy crossing point that connects <b>1</b> and cubane, suggesting that a cycloaddition is theoretically possible. We used the fewest switches surface hopping to study this reaction: 85% of 1,722 trajectories relaxed to 8 products; the major products are bicyclo[4,2,0]octa-2,4,7-triene (30%) and cycloocta-1,3,5,7-tetraene (32%). Only 0.4% of trajectories undergo a [2+2] cycloaddition to form cubane.<i></i></p>


2020 ◽  
Author(s):  
Jingbai Li ◽  
Steven Lopez

<p>Sunlight is a renewable energy source that can be stored in chemical bonds using photochemical reactions. The synthesis of exotic and strained molecules is especially attractive with photochemical techniques because of the associated efficient and mild reaction conditions. We have used complete active space self-consistent field (CASSCF) calculations with an (8,7) active space and the ANO-S-VDZP basis set to understand the photophysics and subsequent photochemistry of a possible cubane precursor tricyclo[4,2,0,0<sup>2,5</sup>]octa-3,7-diene (<b>1</b>). The energies were corrected with a second-order perturbative correction CASPT2(8,7)/ANO-S-VDZP. The S<sub>0</sub>→S<sub>1</sub> vertical excitation energy of <b>1</b> is 6.25 eV, whose nature is π→π<sup>*</sup> excitation. The minimum energy path from the S<sub>1</sub> Franck-Condon point leads directly to a 4π-disrotatory electrocyclic ring-opening reaction to afford bicyclo[4,2,0]octa-2,4,7-triene. The 2D potential energy surface scan located a rhomboidal S<sub>1</sub>/S<sub>0</sub> minimum energy crossing point that connects <b>1</b> and cubane, suggesting that a cycloaddition is theoretically possible. We used the fewest switches surface hopping to study this reaction: 85% of 1,722 trajectories relaxed to 8 products; the major products are bicyclo[4,2,0]octa-2,4,7-triene (30%) and cycloocta-1,3,5,7-tetraene (32%). Only 0.4% of trajectories undergo a [2+2] cycloaddition to form cubane.<i></i></p>


2020 ◽  
Vol 16 (5) ◽  
pp. 3445-3445
Author(s):  
Andrew J. Jenkins ◽  
Hongbin Liu ◽  
Joseph M. Kasper ◽  
Michael J. Frisch ◽  
Xiaosong Li

2009 ◽  
Vol 87 (7) ◽  
pp. 1006-1012 ◽  
Author(s):  
N. Ben Amor ◽  
C. Daniel

The photoinduced homolytic cleavage of the Sn–I bond in iodotrimethylstannane (CH3)3SnI, observed after UV irradiation, is investigated by means of spin–orbit ab initio calculations based on CASSCF (complete active space self-consistent field) and MS-CASPT2 (multi-state complete active space 2nd order perturbation theory) methods. The absorption electronic spectrum is characterized by ten low-lying 1,3A′ and 1,3A″ spin eigenstates corresponding to py(I),px(I) → σ*SnI; σSnI → σ*SnI and py(Sn), px(Sn) → σ*SnI, where σSnI and σ*SnI are the bonding and anti-bonding orbitals of the Sn–I bond along the pz axis. From the 1A′ electronic ground state and these ten spin eigenstates, 21 spin–orbit states are generated leading to various deactivation channels of (CH3)3SnI, corresponding to the formation of radicals (CH3)3Sn• and •I and to the ionic species (CH3)3Sn+ and I–. Irradiation into the upper band at 175 nm should lead to the heterolytic cleavage of the Sn–I bond to form the ionic primary products exclusively, whereas absorption into the shoulder at 250 nm induces the homolytic breaking with formation of the radical products.


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