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1

Szalay, Alexander, John Peacock, Y. Chu L. da Costa, et al. "Commission 47: Cosmology: (Cosmologie)." Transactions of the International Astronomical Union 24, no. 1 (2000): 311–14. http://dx.doi.org/10.1017/s0251107x00003242.

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Abstract (sommario):
Cosmology is one of the most dynamically evolving areas of astrophysics today. Twenty years ago the estimates of the amplitude of the primordial fluctuations were about 10-3, almost a factor of 100 off of today’s measurements. Ten years ago we could only hope for high precision measurements of large scale structure, there were less than 5000 redshifts measured, and only a handful of normal galaxies with z > 1 were known. Computer models of structure formation had just begun to consider non-power-law spectra based on physical models like hot/cold dark matter. As a consequence there was consi
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2

Setti, G., K. Satco, J. Audouze, et al. "Commission 47: Cosmology (Cosmologie)." Transactions of the International Astronomical Union 20, no. 1 (1988): 653–55. http://dx.doi.org/10.1017/s0251107x00007483.

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Abstract (sommario):
The number of pages allocated to the commission report has been very limited and certainly not sufficient to cover in any exhaustive manner the wide range of topics relevant to cosmology and to provide also extensive bibliographies. Because of the vast amount of material to be covered, the report is based on a number of contributions from different colleagues who have been asked to highlight the main trends in the triennium (mid 1984 - mid 1987), together with a list of references sufficiently comprehensive to serve as a guideline for further reading. Unfortunately, two of the expected contrib
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3

Partridge, R. B., V. Trimble, Bernard Fort, et al. "Commission 47: Cosmology (Cosmologie)." Transactions of the International Astronomical Union 22, no. 1 (1994): 539–64. http://dx.doi.org/10.1017/s0251107x00008312.

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4

Peacock, J. A., S. J. Lilly, G. Bruzual, et al. "Commission 47: Cosmology: (Cosmologie)." Transactions of the International Astronomical Union 25, no. 1 (2002): 317–20. http://dx.doi.org/10.1017/s0251107x00001632.

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5

Desmet, Ronny. "La cosmologie de Whitehead [Whitehead’s Cosmology]." Process Studies 37, no. 2 (2008): 200–210. http://dx.doi.org/10.5840/process200837234.

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6

Verde, Licia. "Precision cosmology, Accuracy cosmology and Statistical cosmology." Proceedings of the International Astronomical Union 10, S306 (2014): 223–34. http://dx.doi.org/10.1017/s1743921314013593.

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AbstractThe avalanche of data over the past 10-20 years has propelled cosmology into the “precision era”. The next challenge cosmology has to meet is to enter the era of accuracy. Because of the intrinsic nature of studying the Cosmos and the sheer amount of data available now and coming soon, the only way to meet this challenge is by developing suitable and specific statistical techniques. The road from precision Cosmology to accurate Cosmology goes through statistical Cosmology. I will outline some open challenges and discuss some specific examples.
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7

Steele, Craig. "Cosmology." Journal of Humanistic Mathematics 9, no. 1 (2019): 368. http://dx.doi.org/10.5642/jhummath.201901.26.

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8

Silk, Joseph. "Cosmology." Classical and Quantum Gravity 25, no. 22 (2008): 229003. http://dx.doi.org/10.1088/0264-9381/25/22/229003.

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9

Börner, G. "Cosmology." European Physical Journal Special Topics 152, no. 1 (2007): 139–81. http://dx.doi.org/10.1140/epjst/e2007-00380-7.

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10

Rhee, Jee Sun. "Cosmos, Cosmology and Philosophy of Cosmology: An Essay on Archeology of Cosmology." Journal of The Society of philosophical studies 130 (September 30, 2020): 69–97. http://dx.doi.org/10.23908/jsps.2020.9.130.69.

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11

Spyridon, Melas. "A Selection of Gemstones: Elements of Akbarian Cosmology." Islamovedenie 14, no. 1 (2023): 86–98. http://dx.doi.org/10.21779/2077-8155-2023-14-1-86-98.

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The author notes that the Sufi theological tradition of Akbariya was formed on the basis of the works by Muhyiddin ibn Arabi. Part of this tradition is the doctrine of the nature of the world and its creation, i.e. cosmology. The purpose of the article is to reveal some elements of Akbarian cosmology. The semantic content of the concepts of Akbarian cosmology, creation and approved incarnations is determined. The author maintains that, although things exist eternally, from time immemorial and without beginning in divine knowledge precisely in the form of approved incarnations, at the same time
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12

Thompson, Rodger I. "Testing bound dark energy with cosmological parameter and fundamental constant evolution." Monthly Notices of the Royal Astronomical Society 490, no. 4 (2019): 4778–85. http://dx.doi.org/10.1093/mnras/stz2921.

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ABSTRACT A new bound dark energy (BDE) cosmology has been proposed where the dark energy is the binding energy between light meson fields that condense a few tens of years after the big bang. It is reported that the correct dark energy density emerges using particle physics without fine-tuning. This alone makes the BDE cosmology worthy of further investigation. This work looks at the late-time BDE predictions of the evolution of cosmological parameters and the values of fundamental constants to determine whether the cosmology’s predictions are consistent with observation. The work considers th
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13

Gasperini, M. "String cosmology versus standard and inflationary cosmology." Classical and Quantum Gravity 17, no. 11 (2000): R1—R18. http://dx.doi.org/10.1088/0264-9381/17/11/201.

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14

Apt, Adam J. "Book Review: Keplerian Cosmology, Kepler's Geometrical Cosmology." Journal for the History of Astronomy 20, no. 3 (1989): 213–15. http://dx.doi.org/10.1177/002182868902000305.

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15

Noble, Forrest warrem. "A Clear and Certain Path Replacing the Lambda Cold Dark Matter Model with a More Observationally Verifiable, and Much Less-Problematic Cosmology." European Journal of Applied Physics 5, no. 4 (2023): 10–26. http://dx.doi.org/10.24018/ejphysics.2023.5.4.263.

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At the greatest distances, what James Webb has already observed, and probably will continue to observe based upon our research, is believed by many to be contrary to mainstream cosmology’s predictions concerning the most distant universe. One of the defining differences between the Big Bang model (BB) and prior steady state models (SS) in general was that SS models proposed that the observable universe was unchanging in its general appearance. But an unchanged appearance is what many now believe the James Webb is presently observing. In the decade of the 1960’s, observations were believed to c
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16

Zain, Shaharir Bin Mohd. "The Malayonesian Cosmological Doctrines in Some Past Scientific Writings in Malay." Andalas International Journal of Socio-Humanities 2, no. 1 (2020): 30–49. http://dx.doi.org/10.25077/aijosh.2.1.30-49.2020.

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The Malayonesian cosmological doctrines highlighted here are based on the study of the five Malay inscriptions dated 5th century to 14th century A.D, a traditional Malay folklore on cosmology compiled by Abdullah (1984), and a well known best seller Malay manuscript entitled Taj al-Muluk edited by Syaikh Ismail al-Asyi (1893). We find that the Malayonesian cosmology changes as the people change their religion successively from Hindu to Buddha and to Islam as such that their cosmology became a syncretism of Hindu-Buddha cosmology and Islamic cosmology (after 13th century A.D). But in the second
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17

Zain, Shaharir bin Mohd. "The Malayonesian Cosmological Doctrines in Some Past Scientific Writings in Malay." Andalas International Journal of Socio-Humanities 2, no. 1 (2020): 30–49. http://dx.doi.org/10.25077/aijosh.v2i1.13.

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Abstract (sommario):
The Malayonesian cosmological doctrines highlighted here are based on the study of the five Malay inscriptions dated 5th century to 14th century A.D, a traditional Malay folklore on cosmology compiled by Abdullah (1984), and a well known best seller Malay manuscript entitled Taj al-Muluk edited by Syaikh Ismail al-Asyi (1893). We find that the Malayonesian cosmology changes as the people change their religion successively from Hindu to Buddha and to Islam as such that their cosmology became a syncretism of Hindu-Buddha cosmology and Islamic cosmology (after 13th century A.D). But in the second
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18

Zain, Shaharir bin Mohd. "The Malayonesian Cosmological Doctrines in Some Past Scientific Writings in Malay." Andalas International Journal of Socio-Humanities 2, no. 1 (2020): 30–49. http://dx.doi.org/10.25077/aijosh.v2i1.13.

Testo completo
Abstract (sommario):
The Malayonesian cosmological doctrines highlighted here are based on the study of the five Malay inscriptions dated 5th century to 14th century A.D, a traditional Malay folklore on cosmology compiled by Abdullah (1984), and a well known best seller Malay manuscript entitled Taj al-Muluk edited by Syaikh Ismail al-Asyi (1893). We find that the Malayonesian cosmology changes as the people change their religion successively from Hindu to Buddha and to Islam as such that their cosmology became a syncretism of Hindu-Buddha cosmology and Islamic cosmology (after 13th century A.D). But in the second
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19

Mohammed Sajid Iqbal, Mohammed Sajid Iqbal. "Seven Puzzles for LCDM Cosmology." Indian Journal of Applied Research 3, no. 1 (2011): 91–94. http://dx.doi.org/10.15373/2249555x/jan2013/66.

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20

Moyes, Holley. "Xibalba, the Place of Fear: Caves and the Ancient Maya Underworld." ARYS: Antigüedad, Religiones y Sociedades, no. 14 (May 16, 2018): 171. http://dx.doi.org/10.20318/arys.2017.3990.

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Resumen: Las cuevas eran un elemento destacado de la cosmología maya que encarnaban el inframundo de Xibalba. Como describe el mito, su propio nombre significa “lugar del miedo o el terror”. Aun así, los antiguos mayas se adentraban en la obscuridad de las cavernas para celebrar rituales destinados a divinidades asociadas con la lluvia, la fertilidad, y los ominosos Señores del Inframundo. Aunque se ha escrito poco sobre las prácticas rituales del período maya clásico, los artefactos encontrados en las cuevas documentan que los antiguos mayas dejaron ofrendas de cerámicas, objetos domésticos,
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21

Kanno, Takakazu. "Shinran's Cosmology." JOURNAL OF INDIAN AND BUDDHIST STUDIES (INDOGAKU BUKKYOGAKU KENKYU) 38, no. 1 (1989): 66–68. http://dx.doi.org/10.4259/ibk.38.66.

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22

Pavel, Thomas G., and Vincent Descombes. "Proustian Cosmology." Poetics Today 11, no. 4 (1990): 949. http://dx.doi.org/10.2307/1773083.

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23

D'Amico, Guido, and Nemanja Kaloper. "Rollercoaster cosmology." Journal of Cosmology and Astroparticle Physics 2021, no. 08 (2021): 058. http://dx.doi.org/10.1088/1475-7516/2021/08/058.

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24

McDonald, Michael E. "Scriptural Cosmology." Dialogue: A Journal of Mormon Thought 40, no. 2 (2007): vii—viii. http://dx.doi.org/10.5406/dialjmormthou.40.2.0vii.

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25

Weinstein, Steven. "Romantic cosmology." Physics Today 75, no. 3 (2022): 52–53. http://dx.doi.org/10.1063/pt.3.4964.

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26

Farris, James. "Revisiting Cosmology." Toronto Journal of Theology 18, no. 1 (2002): 101–14. http://dx.doi.org/10.3138/tjt.18.1.101.

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27

Casey, Terence W. "Quantum Cosmology." Physics Essays 3, no. 1 (1990): 89–91. http://dx.doi.org/10.4006/1.3036494.

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28

Blain, A. W., and M. S. Longair. "Submillimetre cosmology." Monthly Notices of the Royal Astronomical Society 264, no. 2 (1993): 509–21. http://dx.doi.org/10.1093/mnras/264.2.509.

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29

FABRIS, JÚLIO C., OLIVER F. PIATTELLA, DAVI C. RODRIGUES, CARLOS E. M. BATISTA, and MAHAMADOU H. DAOUDA. "RASTALL COSMOLOGY." International Journal of Modern Physics: Conference Series 18 (January 2012): 67–76. http://dx.doi.org/10.1142/s2010194512008227.

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We review the difficulties of the generalized Chaplygin gas model to fit observational data, due to the tension between background and perturbative tests. We argue that such issues may be circumvented by means of a self-interacting scalar field representation of the model. However, this proposal seems to be successful only if the self-interacting scalar field has a non-canonical form. The latter can be implemented in Rastall's theory of gravity, which is based on a modification of the usual matter conservation law. We show that, besides its application to the generalized Chaplygin gas model, o
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30

Coley, A. A., and G. F. R. Ellis. "Theoretical cosmology." Classical and Quantum Gravity 37, no. 1 (2019): 013001. http://dx.doi.org/10.1088/1361-6382/ab49b6.

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31

Bassett, Bruce A., David Parkinson, and Robert C. Nichol. "Designer Cosmology." Astrophysical Journal 626, no. 1 (2005): L1—L4. http://dx.doi.org/10.1086/431650.

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32

Zimdahl, Winfried, and Diego Pavón. "Scaling Cosmology." General Relativity and Gravitation 35, no. 3 (2003): 413–22. http://dx.doi.org/10.1023/a:1022369800053.

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33

Stornaiolo, Cosimo. "Tomographic cosmology." Physica Scripta 90, no. 7 (2015): 074032. http://dx.doi.org/10.1088/0031-8949/90/7/074032.

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34

Langlois, David. "Brane Cosmology." Progress of Theoretical Physics Supplement 148 (2002): 181–212. http://dx.doi.org/10.1143/ptps.148.181.

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35

Powell, Corey S. "Goldilocks Cosmology." Scientific American 269, no. 5 (1993): 20–23. http://dx.doi.org/10.1038/scientificamerican1193-20.

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36

Vidotto, Francesca. "Spinfoam Cosmology." Journal of Physics: Conference Series 314 (September 22, 2011): 012049. http://dx.doi.org/10.1088/1742-6596/314/1/012049.

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37

Alvarez, Enrique. "Superstring cosmology." Physical Review D 31, no. 2 (1985): 418–21. http://dx.doi.org/10.1103/physrevd.31.418.

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38

Silk, J. "Holistic Cosmology." Science 277, no. 5326 (1997): 644a—644. http://dx.doi.org/10.1126/science.277.5326.644a.

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39

Karczmarek, Joanna L., and Andrew Strominger. "Matrix Cosmology." Journal of High Energy Physics 2004, no. 04 (2004): 055. http://dx.doi.org/10.1088/1126-6708/2004/04/055.

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40

Wallerstein, George. "Aquinas's Cosmology." Physics Today 40, no. 2 (1987): 134–36. http://dx.doi.org/10.1063/1.2819935.

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41

Zhang, Yuan-Zhong. "Modern Cosmology." Classical and Quantum Gravity 19, no. 12 (2002): 3387–88. http://dx.doi.org/10.1088/0264-9381/19/12/702.

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42

Rajantie, Arttu. "Higgs cosmology." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 376, no. 2114 (2018): 20170128. http://dx.doi.org/10.1098/rsta.2017.0128.

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The discovery of the Higgs boson in 2012 and other results from the Large Hadron Collider have confirmed the standard model of particle physics as the correct theory of elementary particles and their interactions up to energies of several TeV. Remarkably, the theory may even remain valid all the way to the Planck scale of quantum gravity, and therefore it provides a solid theoretical basis for describing the early Universe. Furthermore, the Higgs field itself has unique properties that may have allowed it to play a central role in the evolution of the Universe, from inflation to cosmological p
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43

Chen, P. "Laser cosmology." European Physical Journal Special Topics 223, no. 6 (2014): 1121–29. http://dx.doi.org/10.1140/epjst/e2014-02163-5.

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44

Kehagias, Alexandros A., and Elias Kiritsis. "Mirage cosmology." Journal of High Energy Physics 1999, no. 11 (1999): 022. http://dx.doi.org/10.1088/1126-6708/1999/11/022.

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45

Frankel, Miriam. "Volatile cosmology." New Scientist 264, no. 3518 (2024): 32–35. http://dx.doi.org/10.1016/s0262-4079(24)02075-x.

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46

Hughes, David W. "Considering cosmology." Nature 353, no. 6347 (1991): 804–5. http://dx.doi.org/10.1038/353804b0.

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47

Park, Youngsoo, and Eduardo Rozo. "Concordance cosmology?" Monthly Notices of the Royal Astronomical Society 499, no. 4 (2020): 4638–45. http://dx.doi.org/10.1093/mnras/staa2647.

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ABSTRACT We propose a new intuitive metric for evaluating the tension between two experiments, and apply it to several data sets. While our metric is non-optimal, if evidence of tension is detected, this evidence is robust and easy to interpret. Assuming a flat Lambda cold dark matter (ΛCDM) cosmological model, we find that there is a modest 2.2σ tension between the Dark Energy Survey (DES) Year 1 results and the Planck measurements of the cosmic microwave background. This tension is driven by the difference between the amount of structure observed in the late-time Universe and that predicted
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48

KRANIOTIS, G. V. "STRING COSMOLOGY." International Journal of Modern Physics A 15, no. 12 (2000): 1707–56. http://dx.doi.org/10.1142/s0217751x00000768.

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In this work, we review recent work on string cosmology. The need for an inflationary era is well known. Problems of Standard Cosmology such as horizon, flatness, monopole and entropy find an elegant solution in the inflationary scenario. On the other hand no adequate inflationary model has been constructed so far. In this review we discuss the attempts that have been made in the field of string theory for obtaining an adequate Cosmological Inflationary Epoch. In particular, orbifold compactifications of string theory which are constrained by target-space duality symmetry offer as natural cand
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49

Wong, Jane. "A Cosmology." Massachusetts Review 59, no. 4 (2018): 843–44. http://dx.doi.org/10.1353/mar.2018.0148.

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50

Tzvi Langermann, Y. "Arabic Cosmology." Early Science and Medicine 2, no. 2 (1997): 185–213. http://dx.doi.org/10.1163/157338297x00113.

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AbstractRepresentations of the heavens in various levels of detail can be found in a number of branches of Arabic literature. One particular genre, the hay'a texts, has as its purpose a full though non-mathematical discussion of the arrangement of the celestial orbs; hay'a writers are particularly sensitive to the philosophical requirements which all systems must meet. The pivotal work in this genre, On the Configuration, was written by Ibn al-Haytham. Later writers continued to produce works in the spirit of On the Configuration. In the east, al-Tusi and his followers developed new models; in
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