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Relevant bibliographies by topics / Tolman

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Academic literature on the topic 'Tolman'

Author: Grafiati

Published: 4 June 2021

Last updated: 10 March 2023

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Journal articles on the topic "Tolman"

1

González-Díaz, Pedro F. "Tolman-Hawking kink." Physical Review D 51, no. 12 (1995): 7144–47. http://dx.doi.org/10.1103/physrevd.51.7144.

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Lv, Baozhan, Xiaosong Wang, and Aijun Hu. "Several Theoretical Estimations of Tolman Length." Journal of Computational and Theoretical Nanoscience 13, no. 10 (2016): 6896–900. http://dx.doi.org/10.1166/jctn.2016.5644.

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Based on an analytical formula of the Tolman length, some estimations of the Tolman length were obtained. The Tolman length is non-negative. The Tolman length of the fluid is zero while isothermal compression rate of the fluid is zero. The Tolman length is divergent at the critical point. The curvature dependence of surface tensions of spherical droplets can be further gotten based on this analytical formula of the Tolman length. The surface tensions increase as the radii of spherical droplets increase. Two estimations of the Tolman length are obtained based on Egelstaff–Widom formula and Sanchez’s equation. Based on the results of molecular dynamics simulations, it can be calculated that the value of dimensionless structure constant A of droplets consisted of argon molecular system is 1.9398 when the temperature is 96 K. An estimation of the Tolman length is obtained based on a relationship between the isothermal compressibility, liquid density and speed of sound in a liquid.

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Fau, C., and S. Nabzo. "Tonómetro de Berens-Tolman." Archivos de la Sociedad Española de Oftalmología 94, no. 1 (2019): e4-e5. http://dx.doi.org/10.1016/j.oftal.2018.10.002.

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Rekhviashvili, S. Sh, E. V. Kishtikova, R. Yu Karmokova, and A. M. Karmokov. "Calculating the Tolman constant." Technical Physics Letters 33, no. 1 (2007): 48–50. http://dx.doi.org/10.1134/s1063785007010130.

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Korkina, M. P., and E. M. Kopteva. "Generalization of Tolman–Bondi solution." Astronomical School’s Report 8, no. 1 (2012): 31–33. http://dx.doi.org/10.18372/2411-6602.08.1031.

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Chirinos Isidro, Eddy G., Rodrigo M. Barbosa, Oliver F. Piattella, and Winfried Zimdahl. "Averaged Lemaître–Tolman–Bondi dynamics." Classical and Quantum Gravity 34, no. 3 (2016): 035001. http://dx.doi.org/10.1088/1361-6382/34/3/035001.

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Hellaby, Charles. "Volume matching in Tolman models." General Relativity and Gravitation 20, no. 12 (1988): 1203–17. http://dx.doi.org/10.1007/bf00756049.

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Mackintosh, N. J. "Tolman and modern conditioning theory." British Journal of Psychology 77, no. 4 (1986): 517–23. http://dx.doi.org/10.1111/j.2044-8295.1986.tb02216.x.

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9

González-Diaz, P. F. "On the Tolman-Hawking wormhole." Physical Review D 40, no. 12 (1989): 4184–85. http://dx.doi.org/10.1103/physrevd.40.4184.

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Maharaj, S. D. "On self‐similar Tolman models." Journal of Mathematical Physics 29, no. 6 (1988): 1443–44. http://dx.doi.org/10.1063/1.527938.

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Dissertations / Theses on the topic "Tolman"

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ISIDRO, E. G. C. "Modelos Simples de Lemaitre - Tolman - Bondi (LTB)." Universidade Federal do Espírito Santo, 2015. http://repositorio.ufes.br/handle/10/7459.

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Made available in DSpace on 2018-08-01T22:29:42Z (GMT). No. of bitstreams: 1 tese_8899_Dissertação Eddy Giusepe C. Isidro.pdf: 19967431 bytes, checksum: 09794aab73c65df0a113edc0844e46ae (MD5) Previous issue date: 2015-05-07<br>O modelo padrão atual da cosmologia, o modelo ΛCDM (Λ-Cold Dark Matter), está baseada nas soluções homogêneas de Friedmann-Lemaître-Robertson-Walker (FLRW) das equações de Einstein. As características da Cosmic Microwave Background (CMB) e da formação de estrutura em grandes escalas, são estudadas através da teoria das perturbações cosmológicas no fundo homogêneo e isotrópico. No entanto, nos últimos quinze anos, modelos cosmológicos inomogêneos "simples"que são generalizações do modelo cosmológico FLRW ganharam interesse na comunidade astrofísica e têm sido utilizados para estudar fenômenos cosmológicos. Alguns autores demonstraram que estes modelos inomogêneos com simetria esférica e com fonte de poeira podem reproduzir um bom ajuste para os dados de supernovas do tipo Ia (SNIa) e a posição do primeiro pico da CMB. Estes modelos sugerem que a aparente expansão acelerada do Universo não é causada pela gravidade repulsiva devido à energia escura, mas é sim o resultado das inomogeneidades na distribuição da matéria. Nesta dissertação, os modelos inomogêneos do Universo são investigados na base da métrica de Lemaître-Tolman-Bondi (LTB), o que representa uma solução com simetria esférica para poeira. Dois modelos particulares são estudados: a evolução parabólica com tempo de Big Bang inomogêneo e a evolução hiperbólica com curvatura fraca e tempo de Big Bang constante. As propriedades de cada um destes modelos são investigadas em detalhe, da forma mais analítica possível. Ambos modelos são confrontados com observações astrofísicas da amostra Union2.1 SNIa. Conclui-se que esses modelos podem ser um ponto de partida para desenvolver modelos mais realistas. Portanto, a solução de LTB é capaz de explicar a relação observada entre a distância de luminosidade e o desvio para o vermelho de supernovas sem a necesidade da energia escura quando a inomogeneidade é da forma de um vazio ou quando se tem uma colina centrada no observador com a suposição adicional de que o Universo fora do vazio ou fora da colina é aproximadamente descrito pelo modelo de Einstein-de Sitter homogéneo.

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Gair, Jonathan Reavley. "Generalised Tolman-Bondi cosmologies and Kerr metric atoms." Thesis, University of Cambridge, 2002. https://www.repository.cam.ac.uk/handle/1810/251843.

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In the first part, we derive and investigate a family a cosmological models, which are a generalisation of the Lemaítre-Tolman-Bondi solution. The models are spherically symmetric and are composed of collisionless particles, with each particle possessing angular momentum about the symmetry centre. The radial motion and the magnitude of the angular momentum is the same for every particle on a given spherical shell, but there are particles moving in every tangential direction at each point. In this way the net angular momentum on a given spherical shell is zero and spherical symmetry is maintained. The solution to Einstein's equations describing the family of spacetimes with this matter content is derived in mass and proper time coordinates. The general properties of these models are discussed, including matching conditions and conditions to avoid shell crossing. The self-similar solutions in this family are derived and their physical properties described. A family of radiation spacetimes is obtained by taking the null limit of the particle solutions, i.e. by replacing the particles with photons. These generalize the Vaidya solution. Finally, by taking the limit in which every shell of particle has the same areal radius, a generalisation of the Kantowski-Sachs spacetime is found. These latter solutions may be envisaged as the surface of a cylinder, in which every circular cross section represents a two-sphere. The equation of relative motion of the matter shells along the surface of the cylinder is derived and discussed. The metrics in the general family represent inhomogeneous solutions with only a tangential pressure. This has application as a simple model cosmology or to describe the evolution of regions within our universe, for instance the recollapse of material to form a black hole within an expanding background. The spherical angular momentum model applies to many areas of astrophysics, including the modelling of clusters. These solutions provide a general relativistic description for such situations. The second part of the thesis concerns a problem on the much smaller, atomic scale. The Kerr-Newman solution in general relativity describes the spacetime around a charged and rotating black hole. If the limit <i>G</i> (r) 0 of this solution is taken, flat space is obtained, but the electromagnetic field remains. This electromagnetic field has many interesting properties, and possesses both a charge and magnetic moment. The <i>G</i> (r) 0 limit is appropriate for objects on an atomic scale. In oblate spheroidal coordinates, the Schrödinger equation separates for the electric part of the field, and the Klein-Gordon and Dirac equations separate for the full electromagnetic field. Of particular interest is the latter case, as it describes the interaction of two particles with magnetic moments.

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Elmahalawy, Yasser Reda Ahmed Abdelhamid. "Ricci Time in Lemaître-Tolman Model and Block Universe." Master's thesis, University of Cape Town, 2014. http://hdl.handle.net/11427/13373.

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Includes bibliographical references.<br>It is common to think of our universe according to the "block universe" idea, which says that spacetime consists of many "stacked" 3-surfaces varied as a function of some kind of proper time Ƭ. Standard ideas do not distinguish past and future, but Ellis' "evolving block universe" tries to make a fundamental distinction. One proposal for this proper time is the proper time measured along the timelike Ricci eigenlines, starting from the big bang. The main idea of this work is to investigate the shape of the {Ƭ=constant} surfaces relative to the the null surfaces, and determine what makes these surfaces timelike or spacelike. We use the Lemaître-Tolman metric as our inhomogeneous spacetime model, and we find the necessary and sufficient conditions for these {Ƭ=constant} surfaces to be spacelike or timelike. Furthermore, we indicate whether or not timelike surfaces appear inside black holes and other strong gravity domains, by determining the location of the timelike regions relative to the apparent horizon. Based on this idea, we find that the regions where these surfaces become timelike are often close to the apparent horizons, but always outside them, and in particular timelike regions occur outside black holes. They are always spacelike near the big bang, and at late times (near the crunch or the extreme far future), they are only timelike under special circumstances.

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Leithes, Alexander. "Perturbations in Lemaître-Tolman-Bondi and Assisted Coupled Quintessence cosmologies." Thesis, Queen Mary, University of London, 2017. http://qmro.qmul.ac.uk/xmlui/handle/123456789/24649.

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In this thesis we present research into linear perturbations in Lemaître-Tolman-Bondi (LTB) and Assisted Coupled Quintessence (ACQ) Cosmologies. First we give a brief overview of the standard model of cosmology. We then introduce Cosmological Perturbation Theory (CPT) at linear order for a at Friedmann-Robertson-Walker (FRW) cosmology. Next we study linear perturbations to a Lemaître-Tolman-Bondi (LTB) background spacetime. Studying the transformation behaviour of the perturbations under gauge transformations, we construct gauge invariant quantities in LTB. We show, using the perturbed energy conservation equation, that there is a conserved quantitiy in LTB which is conserved on all scales. We then briefly extend our discussion to the Lemaître spacetime, and construct gauge-invariant perturbations in this extension of LTB spacetime. We also study the behaviour of linear perturbations in assisted coupled quintessence models in a FRW background. We provide the full set of governing equations for this class of models, and solve the system numerically. The code written for this purpose is then used to evolve growth functions for various models and parameter values, and we compare these both to the standard CDM model and to current and future observational bounds. We also examine the applicability of the "small scale approximation", often used to calculate growth functions in quintessence models, in light of upcoming experiments such as SKA and Euclid. We nd the results of the full equations deviates from the approximation by more than the experimental uncertainty for these future surveys. The construction of the numerical code, Pyessence, written in Python to solve the system of background and perturbed evolution equations for assisted coupled quintessence, is also discussed.

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Hickey, Joseph. "Beyond Classical Nucleation Theory: A 2-D Lattice-Gas Automata Model." Thèse, Université d'Ottawa / University of Ottawa, 2012. http://hdl.handle.net/10393/23147.

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Nucleation is the first step in the formation of a new phase in a thermodynamic system. The Classical Nucleation Theory (CNT) is the traditional theory used to describe this phenomenon. The object of this thesis is to investigate nucleation beyond one of the most significant limitations of the CNT: the assumption that the surface tension of a nucleating cluster of the new phase is independent of the cluster’s size and has the same value that it would have in the bulk of the new phase. In order to accomplish this, we consider a microscopic, two-dimensional Lattice Gas Automata (LGA) model of precipitate nucleation in a supersaturated system, with model input parameters Ess (solid particle-to-solid particle bonding energy), Esw (solid particle-to-water particle bonding energy), η (next-to-nearest neighbour bonding coeffiicent in solid phase), and Cin (initial solute concentration). The LGA method was chosen for its advantages of easy implementation, low memory requirements, and fast computation speed. Analytical results for the system’s concentration and the crystal radius as functions of time are derived and the former is fit to the simulation data in order to determine the system’s equilibrium concentration. A mean first-passage time (MFPT) technique is used to obtain the nucleation rate and critical nucleus size from the simulation data. The nucleation rate and supersaturation are evaluated using a modification to the CNT that incorporates a two-dimensional, radius-dependent surface tension term. The Tolman parameter, δ, which controls the radius-dependence of the surface tension, decreases (increases) as a function of the magnitude of Ess (Esw), at fixed values of η and Esw (Ess). On the other hand, δ increases as η increases while Ess and Esw are held constant. The constant surface tension term of the CNT, Σ0, increases (decreases) with increasing magnitudes of Ess (Esw) fixed values of Esw (Ess), and increases as η is increased. Together, these results indicate an increase in the radius-dependent surface tension, Σ, with respect to increasing magnitude of Ess relative to the magnitude of Esw. Σ0 increases linearly as a function of the change in energy during an attachment or detachment reaction, |ΔE|, however with a slope less than that predicted for a crystal that is uniformly packed at maximum density.

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Sobieski, Julian Witold. "Assessing steric bulk of protecting groups via a computational determination of exact cone angle and exact solid cone angle." Kent State University Honors College / OhioLINK, 2018. http://rave.ohiolink.edu/etdc/view?acc_num=ksuhonors1528385706530151.

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Meyer, Sven [Verfasser], and Matthias [Akademischer Betreuer] Bartelmann. "Evolution of linear perturbations in Lemaître-Tolman-Bondi models and effects on light propagation / Sven Meyer ; Betreuer: Matthias Bartelmann." Heidelberg : Universitätsbibliothek Heidelberg, 2015. http://d-nb.info/118049959X/34.

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Ranieri, Domingo. "Modello di universo frattale e accelerazione cosmologica." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/21036/.

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In questo lavoro di tesi mostriamo che l'accelerazione di espansione dell'Universo può essere spiegata senza introdurre un termine di energia oscura ma sfruttando la disomogeneità con cui è distribuita la materia. Diamo una soluzione esatta di un Universo di Lema^itre-Tolman-Bondi (LTB) basato sul presupposto che la metrica ad esso associata sia in grado di descrivere, in media, una distribuzione frattale della materia. Anche se il modello LTB ha un centro, ipotizziamo che, quando la dimensione frattale non è molto diversa dalla dimensione spaziale, questo modello si applichi a qualsiasi punto della struttura frattale che viene scelto come centro. In questo modo, in media, non vi siano punti o direzioni speciali, sfruttando dunque il Principio Cosmologico Condizionale. Utilizzando tale modello esaminiamo la relazione tra modulo di luminosità e redshift dei dati sperimentali delle supernovae di tipo Ia raccolti nel catalogo UNION2. L' analisi mostra che l'apparente accelerazione dell'espansione cosmica può essere interpretata come conseguenza della distribuzione frattale della materia se la sua dimensione frattale ha il valore D = 2,87 +- 0,02 su scale di alcune centinaia di Mpc.

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Marra, Valerio. "A Back-Reaction Approach to Dark Energy." Doctoral thesis, Università degli studi di Padova, 2008. http://hdl.handle.net/11577/3425542.

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This thesis is mainly about how to set up and carry out in a physically meaningful way the idea of back-reaction, which is an alternative theory to a theory where dark energy is fundamental. There are, broadly speaking, two distinct approaches. One is focused on how cosmological observables are affected by inhomogeneities, while the other is focused on a theoretical description of the inhomogeneous universe by means of a mean-field description. Both approaches, however, share the idea of smoothing out inhomogeneities. We developed this duality in the interpretation of the back-reaction by means of toy models based on the Lemaitre-Tolman-Bondi solution of Einstein's equations.

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Karabin, Svyatoslav. "Stelle nel mondo-brana." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2015. http://amslaurea.unibo.it/9566/.

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Lo scopo di questa tesi consiste nello studio delle proprietà generali di sistemi compatti statici e a simmetria sferica nell'ambito dei modelli che prevedono l'esistenza di dimensioni spaziali aggiuntive e che sono comunemente dette del mondo-brana. Si comincerà con una breve descrizione di teorie gravitazionali a più dimensioni, in particolare si parte dalla teoria di Kaluza-Klein, per arrivare ai modelli ADD(Arkani-Hamed, Dimopoulos, Dvali) e infine a quelli RS(Rundall, Sundrum)che interessano direttamente questo studio. Per questi modelli, vengono quindi ricavate le equazioni di campo multidimensionali dall'azione di Einstein-Hilbert e successivamente le si proietta, facendo uso delle equazioni di Gauss e Codazzi, su una brana massiva immersa in un “bulk” cinquedimensionale. Infine si studiano le equazioni di campo di Einstein quadridimensionali per una generica metrica che può servire a descrive stelle statiche, a simmetria sferica e costituite da un fluido perfetto isotropo. Successivamente si ripete la stessa analisi partendo dall'equazione di campo sulla brana e si confrontano i risultati nei due diversi contesti.

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Books on the topic "Tolman"

1

Beek, Wim van der. Ronald Tolman: Sculpturen en etsen. Van Spijk, 1993.

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McLaren, Ian Francis. Henry Tolman Dwight: Bookseller and publisher. University of Melbourne Library, 1989.

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Tolman, F. B. More spit than polish at Tolman Pond. Yankee Books, 1987.

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Donadon, Eleonora. E.C. Tolman e l'epistemologia del primo novecento. Borla, 1997.

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T'aehyŏng, K. Tolmen. Sŏul Munhwasa, 2001.

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Ana, Pogačnik, ed. Tolmin, prazgodovinsko grobišče: Tolmin, the prehistoric cemetery. Narodni muzej Slovenije, 2001.

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Chi, Kŏn-gil, and Hyŏn-jong Cho. Tolsan Songdo. Kungnip Kwangju Pangmulgwan, 1989.

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Brezigar, Inga Miklavčič. Občina Tolmin. Znanstveni inštitut Filozofske fakultete v Ljubljani, 1996.

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Kŏn-gil, Chi, Cho Hyŏn-jong, and Kungnip Kwangju Pangmulgwan, eds. Tolsan Songdo. Kungnip Kwangju Pangmulgwan, 1989.

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Mikʻelaże, Maka. Ixvis tolma. Bakur Sulakauris gamomcʻemloba, 2005.

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Book chapters on the topic "Tolman"

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Vesel, Živa, Leonardo Gariboldi, Steven L. Renshaw, et al. "Tolman, Richard Chace." In The Biographical Encyclopedia of Astronomers. Springer New York, 2007. http://dx.doi.org/10.1007/978-0-387-30400-7_1388.

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Fineburg, Amy C., Catherine Brinckerhoff Jenni, Shuki J. Cohen, et al. "Tolman, E. C." In Encyclopedia of the History of Psychological Theories. Springer US, 2012. http://dx.doi.org/10.1007/978-1-4419-0463-8_122.

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Gale, George. "Tolman, Richard Chace." In Biographical Encyclopedia of Astronomers. Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4419-9917-7_1388.

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Digdon, Nancy. "Edward C. Tolman." In Encyclopedia of Animal Cognition and Behavior. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-47829-6_1692-1.

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Innis, Nancy K. "Tolman, Edward Chace." In Encyclopedia of psychology, Vol. 8. American Psychological Association, 2000. http://dx.doi.org/10.1037/10523-039.

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Digdon, Nancy. "Edward C. Tolman." In Encyclopedia of Animal Cognition and Behavior. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-319-55065-7_1692.

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Lefrancois, Guy R. "Tolman und die Gestaltpsychologie." In Springer-Lehrbuch. Springer Berlin Heidelberg, 1994. http://dx.doi.org/10.1007/978-3-662-12853-4_7.

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Lefrancois, Guy R. "Tolman und die Gestaltpsychologie." In Springer-Lehrbuch. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-662-09577-5_7.

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Seel, Norbert M. "Tolman, Edward C. (1886–1959)." In Encyclopedia of the Sciences of Learning. Springer US, 2012. http://dx.doi.org/10.1007/978-1-4419-1428-6_1841.

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Lefrançois, Guy R. "Übergang zum modernen Kognitivismus: Hebb, Tolman und die Gestaltpsychologen." In Springer-Lehrbuch. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-41972-0_6.

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Conference papers on the topic "Tolman"

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Bochicchio, I., and E. Laserra. "Spherical Tolman-Bondi Models in Cosmology." In Proceedings of the International Conference in Honour of Brian Straughan. WORLD SCIENTIFIC, 2009. http://dx.doi.org/10.1142/9789814293228_0002.

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Mimoso, José P., Alan Maciel, and Morgan Le Delliou. "Tolman-Oppenheimer-Volkov conditions beyond spherical symmetry." In Proceedings of the MG16 Meeting on General Relativity. WORLD SCIENTIFIC, 2023. http://dx.doi.org/10.1142/9789811269776_0197.

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BOCHICCHIO, I. "LEMAÎTRE–TOLMAN–BONDI SOLUTIONS IN f(R)-GRAVITY." In Proceedings of the MG12 Meeting on General Relativity. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814374552_0384.

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Boonserm, Petarpa, Tritos Ngampitipan, and Napasorn Jongjittanon. "Generating Charged Anisotropy and Modified Tolman-Oppenheimer-Volkov Equation." In 6th Annual International Conference on Computational Mathematics, Computational Geometry & Statistics (CMCGS 2017). Global Science & Technology Forum (GSTF), 2017. http://dx.doi.org/10.5176/2251-1911_cmcgs17.21.

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Sussman, Roberto A., Alfredo Macias, and Marco Maceda. "General analytic results on averaging Lemai^tre-Tolman-Bondi models." In RECENT DEVELOPMENTS IN GRAVITATION AND BEC’S PHENOMENOLOGY: IV Mexican Meeting on Experimental and Theoretical Physics: Symposium on Gravitation BEC’s Phenomenology. AIP, 2010. http://dx.doi.org/10.1063/1.3531646.

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Purnamasari, Dian, and Anto Sulaksono. "Energy conditions for neutron stars within parametrized Tolman-Oppenheimer-Volkoff." In CONFERENCE ON THEORETICAL PHYSICS AND NONLINEAR PHENOMENA (CTPNP) 2019: Excursion from Vacuum to Condensed Matter. AIP Publishing, 2020. http://dx.doi.org/10.1063/5.0008136.

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Ai, Xupeng, Zexin Li, Ningyuan Sun, and Xiaoqing Zhu. "Genetic Algorithm Integrated with Neural-Network for Tolman Mouse Robot Navigation." In 2019 IEEE 14th International Conference on Intelligent Systems and Knowledge Engineering (ISKE). IEEE, 2019. http://dx.doi.org/10.1109/iske47853.2019.9170343.

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KRASIŃSKI, ANDRZEJ, and CHARLES HELLABY. "STRUCTURE FORMATION IN THE LEMAîTRE-TOLMAN COSMOLOGICAL MODEL (A NON-PERTURBATIVE APPROACH)." In Proceedings of 2002 International Conference. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812772732_0023.

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Bolvashenkov, I., and H.-G. Herzog. "Highly effective hydrogen production process based on Tolman-Stewart effect: Feasibility of its implementation." In 2013 Eighth International Conference and Exhibition on Ecological Vehicles and Renewable Energies (EVER 2013). IEEE, 2013. http://dx.doi.org/10.1109/ever.2013.6521597.

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Kinreewong, Apisit, Petarpa Boonserm, and Tritos Ngampitipan. "Solution Generating Theorems and Tolman-Oppenheimer-Volkov Equation for Perfect Fluid Spheres in Isotropic Coordinates." In 2016 International Conference on Applied Mathematics, Simulation and Modelling. Atlantis Press, 2016. http://dx.doi.org/10.2991/amsm-16.2016.61.

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Reports on the topic "Tolman"

1

Naranjo Acosta, William Guillermo, Óscar Mauricio Tejada, and José Alejandro Vera Calderón. La curva de Kuznets en el Departamento del Tolima. Universidad Nacional Abierta y a Distancia, 2021. http://dx.doi.org/10.22490/ecacen.5440.

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Abstract:

El presente documento realiza una revisión teórica y empírica de la hipótesis de la curva de Kuznets para el Departamento del Tolima, de acuerdo a la teoría existe una relación empírica entre la desigualdad y el crecimiento económico, en este sentido el siguiente escrito explica la teoría y realiza una contrastación de la hipótesis de Kuznets para el Departamento del Tolima. En primer lugar, se presenta el marco teórico y el estado del arte del fenómeno en estudio, en segundo lugar, se presenta los datos utilizados, y, finalmente, se comprueba la hipótesis en el contexto regional para el Tolima.

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2

Campos-Martínez, Álvaro, Pastor Enrique Quintero-Carvajal, and Álvaro Alberto Ramírez. Evolución y estructura económica y social del Tolima 1980-2002. Banco de la República, 2004. http://dx.doi.org/10.32468/eser.10.

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3

Campos-Martínez, Álvaro. El sector industrial del Tolima : aproximación histórica, estructura y dinámica. Banco de la República, 2004. http://dx.doi.org/10.32468/eser.19.

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4

Quintero-Carvajal, Pastor Enrique, and Jorge Edgar Silva. Tolima : deuda pública municipal con el sector financiero 1994-2003. Banco de la República, 2005. http://dx.doi.org/10.32468/eser.21.

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5

SGC, Servicio Geológico Colombiano. Geología de la plancha 301 Planadas - Departamento del Tolima. Escala 1.100.000. Producto. Versión año 1991. Servicio Geológico Colombiano, 1991. http://dx.doi.org/10.32685/10.143.1991.73.

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6

Gómez, Alberto, Gonzalo Restrepo, Pablo Emilio González-Gómez, and Fernando A. Chalarcá. La industria en el Eje Cafetero y los departamentos de Bolívar, Santander y Tolima 1985-2001. Banco de la República, 2004. http://dx.doi.org/10.32468/eser.15.

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7

SGC, Servicio Geológico Colombiano. Geología de la plancha 303 Colombia. Departamentos de Huila, Tolima y Meta. Escala 1:100.000. Producto. Versión año 2002. Servicio Geológico Colombiano, 2002. http://dx.doi.org/10.32685/10.143.2002.155.

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8

Alturo-Fonseca, Carlos Albeiro, and Carlos Dussán-Pulecio. Contabilidad de gestión en la pequeña empresa manufacturera como herramienta estratégica para la competitividad. Un estudio desde El Espinal (Tolima). Universidad Cooperativa de Colombia, 2016. http://dx.doi.org/10.16925/greylit.1900.

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9

Gómez, Alberto, Pablo Emilio González-Gómez, and Angela María Hurtado. Comportamiento del empleo industrial en Colombia, Eje Cafetero y los departamentos de Bolívar, Santander y Tolima en el periodo 1985-2003. Banco de la República, 2007. http://dx.doi.org/10.32468/eser.42.

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10

Gómez, Alberto, Pablo Emilio González-Gómez, and Felipe Arango. Comportamiento de la inversión en Colombia, el Eje Cafetero y los departamentos de Bolívar, Santander y Tolima en el período 1985-2003. Banco de la República, 2006. http://dx.doi.org/10.32468/eser.43.

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