Info
Vertical teams in the Objective Force [[electronic resource] ] : insights for training and leader development / / James A. Cox ... [and others]
| Vertical teams in the Objective Force [[electronic resource] ] : insights for training and leader development / / James A. Cox ... [and others] |
| Pubbl/distr/stampa | Alexandria, VA : , : U.S. Army Research Institute for the Behavioral and Social Sciences, , [2002] |
| Descrizione fisica | 93 unnumbered pages : digital, PDF file |
| Altri autori (Persone) | CoxJames A |
| Collana | Research report |
| Soggetto topico |
Soldiers - Training of
Vignettes |
| Formato | Materiale a stampa  |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Altri titoli varianti | Vertical teams in the Objective Force |
| Record Nr. | UNINA-9910698777203321 |
| Alexandria, VA : , : U.S. Army Research Institute for the Behavioral and Social Sciences, , [2002] | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Vignettes in gravitation and cosmology [[electronic resource] /] / editors, L. Sriramkumar, T.R. Seshadri
| Vignettes in gravitation and cosmology [[electronic resource] /] / editors, L. Sriramkumar, T.R. Seshadri |
| Pubbl/distr/stampa | Singapore, : World Scientific Pub. Co., 2012 |
| Descrizione fisica | 1 online resource (284 p.) |
| Disciplina |
521.1
523.01 |
| Altri autori (Persone) |
SriramkumarL
SeshadriT. R |
| Soggetto topico |
Gravitation
Cosmology Vignettes |
| Soggetto genere / forma | Electronic books. |
| ISBN | 981-4322-07-5 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
Preface; Contents; 1. Non-linear gravitational clustering in an expanding universe Jasjeet Singh Bagla; 1.1 Introduction; 1.2 Gravitational clustering; 1.2.1 Linear approximation; 1.2.2 Quasi-linear approximations; 1.3 In search of universalities; 1.3.1 Mode coupling: Effect of small scale perturbations; 1.3.2 Mode coupling: Effect of large scale perturbations; 1.4 Conclusions; Acknowledgments; References; 2. Dark ages and cosmic reionization Tirthankar Roy Choudhury; 2.1 Introduction; 2.2 Theoretical formalism; 2.2.1 Cosmological radiation transfer; 2.2.2 Post-reionization epoch
2.2.2.1 Resonant Lyman series absorption2.2.2.2 Continuum absorption; 2.2.3 Pre-overlap epoch; 2.2.4 Reionization of the inhomogeneous IGM; 2.3 Modelling of reionization; 2.3.1 Reionization sources; 2.3.1.1 Mass function of collapsed haloes; 2.3.1.2 Star formation rate; 2.3.1.3 Production of ionizing photons; 2.3.1.4 Feedback processes; 2.3.1.5 Quasars; 2.3.2 Illustration of a semi-analytical model; 2.4 Current status and future; 2.4.1 Simulations; 2.4.2 Various observational probes; 2.4.2.1 Absorption spectra of high redshift sources; 2.4.2.2 CMBR observations; 2.4.2.3 Ly emitters 2.4.2.4 Sources of reionization2.4.2.5 21cm observations; 2.5 Concluding remarks; References; 3. Probing fundamental constant evolution with redshifted spectral lines Nissim Kanekar; 3.1 Introduction; 3.2 Redshifted spectral lines: Background; 3.3 Optical techniques; 3.3.1 The alkali doublet method; 3.3.2 The many-multiplet method; 3.3.3 Molecular hydrogen lines; 3.4 "Radio" techniques; 3.4.1 Radio-optical comparisons; 3.4.2 Radio comparisons; 3.4.3 Ammonia inversion transitions; 3.5 "Conjugate" Satellite OH lines; 3.6 Results from the different techniques; 3.7 Future studies; 3.8 Summary 3.9 AcknowledgmentsReferences; 4. Averaging the inhomogeneous universe Aseem Paranjape; 4.1 Introduction; 4.2 History of the averaging problem; 4.2.1 Noonan's averaging scheme; 4.2.2 Futamase's scheme; 4.2.3 Boersma's scheme; 4.2.4 Kasai's scheme; 4.2.5 Conventional wisdom and controversy; 4.3 Buchert's spatial averaging of scalars; 4.4 Zalaletdinov's Macroscopic Gravity (MG); 4.4.1 A spatial averaging limit; 4.5 Backreaction in cosmological perturbation theory; 4.5.1 Lessons from linear theory; 4.5.2 The nonlinear regime; 4.5.2.1 Dimensional arguments, and why they fail 4.5.3 Calculations in an exact model4.6 Conclusions; 4.6.1 The "Special Observer" assumption; References; 5. Signals of cosmic magnetic fields from the cosmic microwave background radiation T. R. Seshadri; 5.1 Introduction; 5.2 Origin of CMBR; 5.2.1 Homogeneous universe; 5.3 Origin of CMBR and the homogeneity of the universe; 5.4 Finer features of the CMBR: A brief introduction; 5.4.1 Temperature anisotropy; 5.5 Origin of temperature anisotropy in the CMBR; 5.6 Characterizing the nature of CMBR polarization anisotropy; 5.7 Origin of CMBR polarization anisotropy; 5.8 Cosmic magnetic fields 5.9 Polarization in CMBR due to magnetic fields |
| Record Nr. | UNINA-9910451594403321 |
| Singapore, : World Scientific Pub. Co., 2012 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Vignettes in gravitation and cosmology [[electronic resource] /] / editors, L. Sriramkumar, T.R. Seshadri
| Vignettes in gravitation and cosmology [[electronic resource] /] / editors, L. Sriramkumar, T.R. Seshadri |
| Pubbl/distr/stampa | Singapore, : World Scientific Pub. Co., 2012 |
| Descrizione fisica | 1 online resource (284 p.) |
| Disciplina |
521.1
523.01 |
| Altri autori (Persone) |
SriramkumarL
SeshadriT. R |
| Soggetto topico |
Gravitation
Cosmology Vignettes |
| ISBN | 981-4322-07-5 |
| Formato | Materiale a stampa |
| Livello bibliografico | Monografia |
| Lingua di pubblicazione | eng |
| Nota di contenuto |
Preface; Contents; 1. Non-linear gravitational clustering in an expanding universe Jasjeet Singh Bagla; 1.1 Introduction; 1.2 Gravitational clustering; 1.2.1 Linear approximation; 1.2.2 Quasi-linear approximations; 1.3 In search of universalities; 1.3.1 Mode coupling: Effect of small scale perturbations; 1.3.2 Mode coupling: Effect of large scale perturbations; 1.4 Conclusions; Acknowledgments; References; 2. Dark ages and cosmic reionization Tirthankar Roy Choudhury; 2.1 Introduction; 2.2 Theoretical formalism; 2.2.1 Cosmological radiation transfer; 2.2.2 Post-reionization epoch
2.2.2.1 Resonant Lyman series absorption2.2.2.2 Continuum absorption; 2.2.3 Pre-overlap epoch; 2.2.4 Reionization of the inhomogeneous IGM; 2.3 Modelling of reionization; 2.3.1 Reionization sources; 2.3.1.1 Mass function of collapsed haloes; 2.3.1.2 Star formation rate; 2.3.1.3 Production of ionizing photons; 2.3.1.4 Feedback processes; 2.3.1.5 Quasars; 2.3.2 Illustration of a semi-analytical model; 2.4 Current status and future; 2.4.1 Simulations; 2.4.2 Various observational probes; 2.4.2.1 Absorption spectra of high redshift sources; 2.4.2.2 CMBR observations; 2.4.2.3 Ly emitters 2.4.2.4 Sources of reionization2.4.2.5 21cm observations; 2.5 Concluding remarks; References; 3. Probing fundamental constant evolution with redshifted spectral lines Nissim Kanekar; 3.1 Introduction; 3.2 Redshifted spectral lines: Background; 3.3 Optical techniques; 3.3.1 The alkali doublet method; 3.3.2 The many-multiplet method; 3.3.3 Molecular hydrogen lines; 3.4 "Radio" techniques; 3.4.1 Radio-optical comparisons; 3.4.2 Radio comparisons; 3.4.3 Ammonia inversion transitions; 3.5 "Conjugate" Satellite OH lines; 3.6 Results from the different techniques; 3.7 Future studies; 3.8 Summary 3.9 AcknowledgmentsReferences; 4. Averaging the inhomogeneous universe Aseem Paranjape; 4.1 Introduction; 4.2 History of the averaging problem; 4.2.1 Noonan's averaging scheme; 4.2.2 Futamase's scheme; 4.2.3 Boersma's scheme; 4.2.4 Kasai's scheme; 4.2.5 Conventional wisdom and controversy; 4.3 Buchert's spatial averaging of scalars; 4.4 Zalaletdinov's Macroscopic Gravity (MG); 4.4.1 A spatial averaging limit; 4.5 Backreaction in cosmological perturbation theory; 4.5.1 Lessons from linear theory; 4.5.2 The nonlinear regime; 4.5.2.1 Dimensional arguments, and why they fail 4.5.3 Calculations in an exact model4.6 Conclusions; 4.6.1 The "Special Observer" assumption; References; 5. Signals of cosmic magnetic fields from the cosmic microwave background radiation T. R. Seshadri; 5.1 Introduction; 5.2 Origin of CMBR; 5.2.1 Homogeneous universe; 5.3 Origin of CMBR and the homogeneity of the universe; 5.4 Finer features of the CMBR: A brief introduction; 5.4.1 Temperature anisotropy; 5.5 Origin of temperature anisotropy in the CMBR; 5.6 Characterizing the nature of CMBR polarization anisotropy; 5.7 Origin of CMBR polarization anisotropy; 5.8 Cosmic magnetic fields 5.9 Polarization in CMBR due to magnetic fields |
| Record Nr. | UNINA-9910779278503321 |
| Singapore, : World Scientific Pub. Co., 2012 | ||
| Materiale a stampa | ||
| Lo trovi qui: Univ. Federico II | ||
| ||
Soggetto topico
-
Vignettes
(3)
- Cosmology (2)
- Gravitation (2)
- Soldiers - Training of (1)