Elements of Astrochemistry: Chemical History of Matter in the Universe

In the last half-century, financial derivatives have become progressively central in finance being actively traded on many exchanges throughout the world and entered into by financial institutions, fund managers, and corporate treasurers. Elements of Financial Mathematics: From Interest Theory to Options book presents those mathematical models that continue to reveal essentials for understanding the relationships among the actors in the financial world: annuities, bonds, portfolio theory, and derivatives. Cover Copyright DECLARATION ABOUT THE EDITOR TABLE OF CONTENTS List of Contributors List of Abbreviations Preface Section 1: The Measurement of the Universe by Spectroscopy Chapter 1 Remote Sensing of Exoplanetary Atmospheres with Ground-Based High-Resolution Near-Infrared Spectroscopy Abstract Introduction Methods Validation of The Method Results Suggested Observation Strategies and Potential Targets Discussion Summary References Chapter 2 Broadband Spectroscopy of Astrophysical ICE Analogues Abstract Introduction Experimental And Theoretical Methods Derivation of The Optical Constants Discussion Conclusions Acknowledgments Appendix A: Thz-Tds Optics Appendix B: Reconstruction Of The Terahertz Dielectric Permittivity Appendix C: Opacity Model Benchmark References Section 2: From the Very Early Universe to the First Atoms Chapter 3 Big Bang Nucleosynthesis in Visible and Hidden-Mirror Sectors Abstract Introduction Models Results Conclusions References Chapter 4 Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles Abstract Introduction Observed Abundances Of Light Elements Bbn With Decaying Particles Constraints On Generic Decaying Particles Constraints On Various Decay Modes Gravitino Conclusions And Discussion References Section 3: Stars and the Creation of the Higher Elements Chapter 5 Formation of the First Stars in the Universe Abstract Introduction: The Dark Ages Hierarchical Structure Formation And The First Cosmological Objects Formation of The First Cosmological Objects The Role of Dark Matter And Dark Energy Formation of The First Stars The Mass of The First Stars Feedback From The First Stars Formation of The First Galaxies And Black Holes Prospects For Future Observations Acknowledgements Appendix A: Density Fluctuations And Mass Variance References Chapter 6 Observational Constraints on the Origin of the Elements I. 3D NLTE formation of Mn lines in late-type Stars Abstract Introduction Observations Analysis Results 1D NLTE 3D NLTE Solarmn Abundance 3D NLTE Effects In Metal-Poor Model Atmospheres 3D LTE Versus 3D NLTE Benchmark Metal-Poor Stars Conclusions Acknowledgements Appendix A Additional Figures Appendix B Additional Tables References Section 4: Interstellar Chemistry Chapter 7 H2 Formation on Interstellar Dust Grains: The Viewpoints of Theory, Experiments, Models and Observations Abstract Introduction State Of The Art Recommended Parameters H2 Formation In Different Astrophysical Environments Conclusions And Perspectives Acknowledgements References Chapter 8 The First Steps of Interstellar Phosphorus Chemistry Abstract Introduction Observations Results Chemical Modeling Discussion: The Chemistry Of Phosphorus Future Observations Conclusions Acknowledgements Appendix A The Depletion Of Phosphorus References Section-5: Laboratory-Based Astrochemistry Chapter 9 Grain Surface Models and Data for Astrochemistry Abstract Introduction Outline Of A Generic Gas-Grain Code Accretion Desorption Reactive/Chemical Desorption Reactions Tunneling Diffusion Bulk Processes Precision Considerations In Rate-Based Modeling Outlook References Chapter 10 Experimental Study of the Penetration of Oxygen and Deuterium Atoms into Porous Water ICE Abstract Introduction Experimental Methods Experimental Results Model And Discussion Astrophysical Implications And Conclusions Acknowledgements References Section 6: Chemistry of the Solar System Chapter 11 Constraining the Evolutionary History of the Moon and the Inner Solar System: A Case for New Returned Lunar Samples Abstract Overview Of Our Lunar Sample Collection When Did The Moon Form? Petrology And Formation History Of The Lunar Anorthositic Crust The Bombardment History Of The Inner Solar System Nature, Timing, And Duration Of Lunar Mare Volcanism Structure And Composition Of The Lunar Interior Icy Deposits At The Lunar Poles The Lunar Regolith As A Recorder Of The Sun’s Composition, Activity And Galactic Environment The Lunar Magnetic Field Summary Notes References Chapter 12 Silica-rich Volcanism in the Early Solar System Dated at 4.565 Ga Abstract Introduction Results Discussion Methods References Index Back Cover