Relevant bibliographies by topics / Inflation,Primordial Black Holes

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Inflation,Primordial Black Holes'

Author: Grafiati
Published: 27 July 2021
Last updated: 8 February 2022

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Journal articles on the topic "Inflation,Primordial Black Holes"

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Dimopoulos, Konstantinos, Tommi Markkanen, Antonio Racioppi, and Ville Vaskonen. "Primordial black holes from thermal inflation." Journal of Cosmology and Astroparticle Physics 2019, no. 07 (July 31, 2019): 046. http://dx.doi.org/10.1088/1475-7516/2019/07/046.

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Cicoli, Michele, Victor A. Diaz, and Francisco G. Pedro. "Primordial black holes from string inflation." Journal of Cosmology and Astroparticle Physics 2018, no. 06 (June 25, 2018): 034. http://dx.doi.org/10.1088/1475-7516/2018/06/034.

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POLARSKI, D. "CLASSICALITY OF PRIMORDIAL FLUCTUATIONS AND PRIMORDIAL BLACK HOLES." International Journal of Modern Physics D 10, no. 06 (December 2001): 927–34. http://dx.doi.org/10.1142/s021827180100161x.

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The production of Primordial Black Holes (PBH) from inflationary perturbations provides a physical process where the effective classicality of the fluctuations does not hold for certain scales. For adiabatic perturbations produced during inflation, this range of scales corresponds to PBH with masses M≪1015 g. For PBH with masses M ~ M H (te), the horizon mass at the end of inflation, the generation process during the preheating stage could be classical as well, in contrast to the formation of PBH on these scales by adiabatic inflationary perturbations. For the nonevaporated PBH, the generation process is essentially classical.
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Kamenshchik, Alexander Y., Alessandro Tronconi, Tereza Vardanyan, and Giovanni Venturi. "Non-canonical inflation and primordial black holes production." Physics Letters B 791 (April 2019): 201–5. http://dx.doi.org/10.1016/j.physletb.2019.02.036.

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Conzinu, P., M. Gasperini, and G. Marozzi. "Primordial black holes from pre-big bang inflation." Journal of Cosmology and Astroparticle Physics 2020, no. 08 (August 13, 2020): 031. http://dx.doi.org/10.1088/1475-7516/2020/08/031.

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Arya, Richa. "Formation of primordial black holes from warm inflation." Journal of Cosmology and Astroparticle Physics 2020, no. 09 (September 21, 2020): 042. http://dx.doi.org/10.1088/1475-7516/2020/09/042.

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Ivanov, P., P. Naselsky, and I. Novikov. "Inflation and primordial black holes as dark matter." Physical Review D 50, no. 12 (December 15, 1994): 7173–78. http://dx.doi.org/10.1103/physrevd.50.7173.

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Drees, Manuel, and Encieh Erfani. "Running-mass inflation model and primordial black holes." Journal of Cosmology and Astroparticle Physics 2011, no. 04 (April 5, 2011): 005. http://dx.doi.org/10.1088/1475-7516/2011/04/005.

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Kannike, K., L. Marzola, M. Raidal, and H. Veermäe. "Single field double inflation and primordial black holes." Journal of Cosmology and Astroparticle Physics 2017, no. 09 (September 12, 2017): 020. http://dx.doi.org/10.1088/1475-7516/2017/09/020.

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Pattison, Chris, Vincent Vennin, Hooshyar Assadullahi, and David Wands. "Quantum diffusion during inflation and primordial black holes." Journal of Cosmology and Astroparticle Physics 2017, no. 10 (October 26, 2017): 046. http://dx.doi.org/10.1088/1475-7516/2017/10/046.

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Dissertations / Theses on the topic "Inflation,Primordial Black Holes"

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Zucchini, Sara. "Primordial black holes in string inflation." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/17097/.

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In this thesis we consider the production of primordial black holes (PBH) in the context of single field inflation with the aim of describing a significant fraction of dark matter. In the models we consider, the inflaton is a string modulus and its potential is typical of type IIB fibre inflation. The potential presents a plateau at CMB scales and an extremely flat region on smaller scales. The background is analysed by solving the Friedmann's and the Klein-Gordon equations for the system. Perturbations are introduced through the usual Mukhanov-Sasaki equation for the gauge invariant curvature perturbations, whose solution allows us to find the primordial power spectrum which is then compared to observations. In the class of models considered there is an often occurring tension between the tilt of the scalar power spectrum and observations. We study this tension and propose mechanisms to minimise it. We modify the form of the fibre inflationary potential, modifying therefore the slope of the ultra slow-roll plateau. We find that a better agreement with the experimentally measured value of the spectral index can be reached. Therefore that tension between the value of the spectral index on CMB scale and the power spectrum enhancement on PBH scales can be explained as a consequence of the class of potential taken into account. This tension can be avoided in models that provide a different plateau form.
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Pedrelli, Luca. "Inflation and primordial black holes in matter domination." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/17095/.

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In this thesis we will study a new interpretation of dark matter in terms of Primordial Black Holes (PBHs), i.e. black holes that are believed to form when large density perturbations, produced during the inflationary epoch, reenter the horizon and collapse because of their own gravitational force. Black holes produced in this way are referred to as "Primordial" since their production mechanism has a primordial origin during inflation. These large density fluctuations are produced if the inflationary potential possesses enough tuning freedom to feature a slow-roll plateau followed by a near inflection point that greatly enhances the power spectrum of scalar perturbations. We examine PBH formation during a radiation dominated (RD) epoch and during a matter dominated (MD) epoch driven by a gravitationally coupled scalar field (modulus) which decays before Big Bang Nucleosynthesis in order to preserve its successful predictions. We will require in both cases that the produced PBHs constitute 100% of dark matter today. In the MD case, we find that the mass of the scalar field affects the enhancement required in the curvature power spectrum: for large modulus masses, this enhancement turns out to be smaller than the one in the RD case, meaning that in the case of horizon reentry during moduli domination the potential requires less tuning to produce the same amount of PBHs. Therefore, we focus on PBH production during a MD epoch. We then introduce a model of string inflation called "Fibre Inflation", that works particularly well for our purposes since it naturally leads to a post-inflationary epoch of MD driven by an axion-like modulus. In this model the inflationary potential has enough tuning freedom to induce a period of ultra slow-roll that enhances the density perturbations at the required PBH scales: we employ this potential to obtain a numerical estimate of the scalar power spectrum and the other inflationary observables.
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Copparoni, Lorenzo. "Generating primordial black holes in non-canonical inflation." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/23537/.

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Among the candidates for dark matter, Primordial Black Holes are extremely promising, as they do not require the introduction of new physics beyond the Standard Model of particle physics. These objects can arise from the collapse of overdense regions generated by the curvature perturbation generated during inflation. The probability distribution of these overdense regions is related to the power spectrum of the scalar perturbation which must be enhanced by compared to the perturbation at CMB scale in order for the collapse to generate enough Primordial Black Holes to account for the dark mater budget we observe today. In this thesis we discuss two possible amplification mechanism in non-canonical inflation, employing a decreasing sound speed. In the first case we consider a model which starts in a slow-roll regime at CMB scale. Later during inflation the field enters in a non-canonical regime and it approaches the k-inflation attractor. During this kinetically driven transient phase the sound speed and the slow roll parameter $\epsilon$ decrease exponentially and the power spectrum of the curvature perturbation gets amplified. We then consider a DBI model where we consider the presence of a gaussian spike in the warp factor, thus leading to the transition, from the canonical phase at CMB scales to a strongly non-canonical regime. In this latter phase, the sound speed of perturbation is much smaller than 1, and leads to an amplification of the scalar perturbation power spectrum.
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Erfani, Encieh [Verfasser]. "Inflation and Dark Matter Primordial Black Holes / Encieh Erfani." Bonn : Universitäts- und Landesbibliothek Bonn, 2012. http://d-nb.info/104408250X/34.

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Pedron, Nicola. "Gravitational waves from primordial black holes in string inflation." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/23236/.

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We consider a model of inflation, called Fibre Inflation, derived from string theory in the framework of type IIB flux compactification and we study the production of primordial black holes due to the gravitational collapse of the curvature perturbations. They are a good candidate for dark matter and if their mass was between 10^-17 and 10^-13 solar masses then their contribution to the total dark matter abundance would be between 10% and 100%. The inflaton potential has enough tuning freedom to allow for a flat plateau at large field values, corresponding to the usual slow roll behaviour, and an inflection point near the minimum that enhances the scalar perturbations. It is the latter feature that greatly increases the density anisotropies from the usual δρ/ρ ~ 10^-5, typical of the CMB radiation, to δρ/ρ ~ 10^-1 due to a peak in the primordial power spectrum that allows for the formation of black holes. The latter is computed solving the Mukhanov-Sasaki equation numerically using the Hubble slow roll parameters extracted from the solutions to the Friedmann equations and the inflaton equation of motion. The formation of black holes is followed by the production of a stochastic background of secondary gravitational waves: in this thesis we compute their amplitude and compare it with current observational bounds and the sensitivities of earth- and space-based interferometers. Our result is within reach of experiments like DECIGO and BBO, hence in the future it will be possible to have a comparison between our theoretical results and observations.
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Green, Anne M. "Constraining models of the early universe : inflation, primordial black holes and cosmic strings." Thesis, University of Sussex, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.263155.

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Giguere, Alexis. "Primordial black hole seeding from hybrid inflation : the direct integration approach." Thesis, Massachusetts Institute of Technology, 2013. http://hdl.handle.net/1721.1/88905.

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Thesis: S.B., Massachusetts Institute of Technology, Department of Physics, 2013.
Cataloged from PDF version of thesis.
Includes bibliographical references (page 45).
We examine the notion that supermassive black holes at the centre of galaxies, such as the Milky Way, could have been seeded in the early universe by the mechanisms of hybrid inflation. Using luminosity data, we estimate the current density of supermassive black hole. We develop the formalism of the dierct integration method in hybrid inflation and obtain a power spectrum, which we try to relate to the literature. Our results do not directly show the plausibility of seeding supermassive black holes, but the shape of the power spectrum suggests that further work might yield positive results.
by Alexis Giguere.
S.B.
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Longo, Mirko. "Stochastic effects in ultra slow-roll inflation." Master's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/17098/.

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In this work we apply the stochastic inflation formalism to backgrounds that deviate from standard slow-roll in a way that can lead to the production of primordial black holes. We analyse the effects of sudden transitions on the stochastic noise amplitude and its potential impact on the production of primordial black holes in single field inflation. We justify the claim that primordial black holes can be responsible for a significant fraction of the dark matter abundance today and estimate the required enhancement in the power spectrum. We introduce the Hamiltonian formalism and the coarse-graining of the quantum field and its momentum, allowing us to obtain a quantitative measure of the role of quantum diffusion in the production of primordial black holes. We mainly focus our analysis on a Starobinsky potential given that it is rich enough to allow for the dynamics of the scalar field during inflation to include an ultra slow-roll phase induced by a transition from a relatively large slow-roll parameter to a hierarchically smaller one. This has the effect of making the field perturbations undergo sudden transitions and rise from its ground state to an excited state. We present two procedures that we employed when calculating the power spectrum: a numerical and an analytical one. Both methods show that stochastic effects are negligible at small scales where their amplitude is time dependent and vanishes at late times, and that for scales leaving the horizon after the ultra slow-roll phase the de Sitter estimate of $H^2/(4\pi^2)$ is approximately correct. We therefore demonstrate that the estimates in the literature are incomplete and that a revaluation of the role of stochastic effects on primordial black hole production is in order.
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Martineau, Killian. "Quelques aspects de cosmologie et de physique des trous noirs en gravitation quantique à boucles Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi I universe with different inflaton potentials and initial conditions Some clarifications on the duration of inflation in loop quantum cosmology A first step towards the inflationary trans-Planckian problem treatment in loop quantum cosmology Scalar spectra of primordial perturbations in loop quantum cosmology Phenomenology of quantum reduced loop gravity in the isotropic cosmological sector Primordial Power Spectra from an Emergent Universe: Basic Results and Clarifications Fast radio bursts and the stochastic lifetime of black holes in quantum gravity Quantum fields in the background spacetime of a polymeric loop black hole Quasinormal modes of black holes in a toy-model for cumulative quantum gravity Seeing through the cosmological bounce: Footprints of the contracting phase and luminosity distance in bouncing models Dark matter as Planck relics without too exotic hypotheses A Status Report on the Phenomenology of Black Holes in Loop Quantum Gravity: Evaporation, Tunneling to White Holes, Dark Matter and Gravitational Waves." Thesis, Université Grenoble Alpes (ComUE), 2019. http://www.theses.fr/2019GREAY044.

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Cantonnée à la physique mathématique depuis des décennies, la gravitation quantique entre désormais dans le giron de la science expérimentale. Suivant cette mouvance nous considérons dans cette thèse trois cadres d’application de la gravitation quantique à boucles (LQG) : le système Univers, les trous noirs et les astroparticules. Le troisième n’est qu’esquissé tandis que les deux premiers sont présentés plus en détails.Le secteur cosmologique étant l’un des domaines les plus prometteurs pour tester et contraindre des théories de gravité quantique, le développement de différents modèles tentant d’appliquer les idées de la LQG à l’Univers primordial ne s’est pas fait attendre. Les travaux que nous présentons portent sur la phénoménologie associée à ces modèles; tant dans le secteur homogène (où nous nous focalisons notamment sur la durée de la phase d’inflation), que dans le secteur inhomogène (nous étudions ce coup-ci le devenir des spectres de puissance primordiaux). Ces études combinées nous permettent alors de préciser dans quelle mesure des effets de gravité quantique (à boucles) peuvent être observés dans les anisotropies du fond diffus cosmologique.D’autre part les trous noirs, non contents de faire partie des objets les plus étranges et les plus fascinants de l’Univers, constituent également des sondes privilégiées pour tester des théories de gravitation. Nous développons la phénoménologie associée à différents traitements des trous noirs en gravitation quantique à boucles. Celle-ci intervient sur une grande variété de fronts : de l’évaporation de Hawking aux ondes gravitationnelles, en passant par la matière noire. C’est sans nul doute un domaine riche et vaste.Finalement, l’existence d’une échelle de longueur minimale, prédite par la majorité des théories de gravité quantique, suggère une généralisation du principe d’incertitude de Heisenberg. Partant de ce constat nous présentons également dans ce manuscrit une méthodologie permettant de calculer une nouvelle relation de dispersion de la lumière à partir du principe d’incertitude généralisé le plus couramment répandu
After decades of being confined to mathematical physics, quantum gravity now enters the field of experimental science. Following this trend, we consider throughout this thesis three implementation frameworks of Loop Quantum Gravity (LQG): the Universe as a system, black holes and astroparticles. The last one is only outlined while the first two are presented in more detail.Since the cosmological sector is one of the most promising areas for testing and constraining quantum gravity theories, it was not long before the development of different models attempting to apply the ideas of the LQG to the primordial Universe. The work we present deals with the phenomenology associated with these models; both in the homogeneous sector (where we focus particularly on the duration of the inflation phase), as in the inhomogeneous sector (where this time, we study the fate of the primordial power spectra). These combined studies then allow us to specify to what extent effects of (loop) quantum gravity can be observed in the anisotropies of the cosmic microwave background.On the other hand black holes, not content to be among the strangest and most fascinating objects of the Universe, are also prominent probes to test the theories of gravitation. We develop the phenomenology associated with different treatments of black holes in the loop quantum gravity framework, which intervenes on multiple levels: from the evaporation of Hawking to gravitational waves, including dark matter. This is undoubtedly a rich and vast area.Finally, the existence of a minimal length scale, predicted by the majority of quantum gravity theories, suggests a generalization of the Heisenberg uncertainty principle. On the basis of this observation, we also present in this manuscript a methodology to derive a new relation dispersion of light from the most widely used generalized uncertainty principle
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MacGibbon, Jane Helena. "Quark and gluon evaporation from primordial black holes." Thesis, University of Cambridge, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.279714.

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Books on the topic "Inflation,Primordial Black Holes"

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Quantum theory, black holes, and inflation. Chichester: Wiley, 1996.

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Hawkins, Michael. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. Reading, Mass: Addison-Wesley, 1997.

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Celia, Fitzgerald, ed. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. Reading, Mass: Perseus Books, 1998.

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Michael, Hawkins. Hunting down the universe: The missing mass, primordial black holes, and other dark matters. London: Little, Brown, 1997.

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Maggiore, Michele. Gravitational Waves. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198570899.001.0001.

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A comprehensive and detailed account of the physics of gravitational waves and their role in astrophysics and cosmology. The part on astrophysical sources of gravitational waves includes chapters on GWs from supernovae, neutron stars (neutron star normal modes, CFS instability, r-modes), black-hole perturbation theory (Regge-Wheeler and Zerilli equations, Teukoslky equation for rotating BHs, quasi-normal modes) coalescing compact binaries (effective one-body formalism, numerical relativity), discovery of gravitational waves at the advanced LIGO interferometers (discoveries of GW150914, GW151226, tests of general relativity, astrophysical implications), supermassive black holes (supermassive black-hole binaries, EMRI, relevance for LISA and pulsar timing arrays). The part on gravitational waves and cosmology include discussions of FRW cosmology, cosmological perturbation theory (helicity decomposition, scalar and tensor perturbations, Bardeen variables, power spectra, transfer functions for scalar and tensor modes), the effects of GWs on the Cosmic Microwave Background (ISW effect, CMB polarization, E and B modes), inflation (amplification of vacuum fluctuations, quantum fields in curved space, generation of scalar and tensor perturbations, Mukhanov-Sasaki equation,reheating, preheating), stochastic backgrounds of cosmological origin (phase transitions, cosmic strings, alternatives to inflation, bounds on primordial GWs) and search of stochastic backgrounds with Pulsar Timing Arrays (PTA).
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Vigdor, Steven E. The Dark Side. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814825.003.0006.

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Chapter 6 deals with the remaining mysteries in cosmology—dark matter, dark energy, and inflationary expansion—and the experiments aimed at solving them. It reviews the evidence for dark matter, and experiments to detect the microscopic particles proposed as its constituents: weakly interacting massive particles and invisible axions. Contrasts are drawn between the failure to understand the scale of dark energy theoretically and the ambitious new survey telescopes, such as the Large Synoptic Survey Telescope (or LSST), that aim to constrain its equation of state. The theoretical concepts and possible experimental signatures of cosmic inflation are described. Searches for possible imprints from primordial inflation-induced gravitational waves on the polarization of the cosmic microwave background (CMB polarization) are discussed in the context of the pioneering first detection by the Laser Interferometer Gravitational-Wave Observatory (or LIGO) of gravitational waves from distant black-hole mergers. Philosophical questions regarding the falsifiability of inflation are raised.
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HAWKINS, MICHAEL. HUNTING DOWN THE UNIVERSE: THE MISSING MASS, PRIMORDIAL BLACK HOLES AND OTHER DARK MATTERS. ABACUS, 1998.

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Kachelriess, Michael. Quantum Fields. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198802877.001.0001.

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This book introduces quantum field theory, together with its most important applications to cosmology and astroparticle physics, in a coherent framework. The path-integral approach is employed right from the start, and the use of Green functions and generating functionals is illustrated first in quantum mechanics and then in scalar field theory. Massless spin one and two fields are discussed on an equal footing, and gravity is presented as a gauge theory in close analogy with the Yang–Mills case. Concepts relevant to modern research such as helicity methods, effective theories, decoupling, or the stability of the electroweak vacuum are introduced. Various applications such as topological defects, dark matter, baryogenesis, processes in external gravitational fields, inflation and black holes help students to bridge the gap between undergraduate courses and the research literature.
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Book chapters on the topic "Inflation,Primordial Black Holes"

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Arya, Richa. "Primordial Black Holes from Warm Inflation." In Springer Proceedings in Physics, 67–73. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-6292-1_8.

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Calmet, Xavier, Bernard Carr, and Elizabeth Winstanley. "Primordial Black Holes." In SpringerBriefs in Physics, 51–81. Berlin, Heidelberg: Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-38939-9_4.

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Kapusta, Joseph I. "Primordial Black Holes and Hot Matter." In Phase Transitions in the Early Universe: Theory and Observations, 471–81. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0997-3_21.

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Carr, Bernard J. "Primordial Black Holes and Quantum Effects." In Springer Proceedings in Physics, 23–31. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-20046-0_3.

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Jedamzik, Karsten. "Primordial Black Holes as Dark Matter." In Dark Matter in Astro- and Particle Physics, 289–96. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1_27.

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Novikov, Igor D., and Valery P. Frolov. "Primordial Black Holes and the Ultimate Fate of Black and White Holes." In Physics of Black Holes, 288–301. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-017-2651-1_13.

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Arai, Kenzo, Masa-aki Hashimoto, and Toshifumi Futamase. "Primordial Black Holes and Big Bang Nucleosynthesis." In Primordial Nucleosynthesis and Evolution of Early Universe, 65–66. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3410-1_9.

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Vidotto, F., A. Barrau, B. Bolliet, M. Schutten, and C. Weimer. "Quantum-Gravity Phenomenology with Primordial Black Holes." In Springer Proceedings in Physics, 157–63. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-94256-8_18.

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Roest, Diederik, and Marco Scalisi. "Inflation: Observations and Attractors." In Theoretical Frontiers in Black Holes and Cosmology, 221–49. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-31352-8_6.

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Green, Anne M. "Primordial Black Holes: Sirens of the Early Universe." In Fundamental Theories of Physics, 129–49. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10852-0_5.

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Conference papers on the topic "Inflation,Primordial Black Holes"

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RUBIN, S. G. "MASSIVE PRIMORDIAL BLACK HOLES IN HYBRID INFLATION." In Proceedings of the International Conference. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702883_0038.

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Ketov, Sergei V. "Inflation, primordial black holes and induced gravitational waves from modified supergravity." In 1st Electronic Conference on Universe. Basel, Switzerland: MDPI, 2021. http://dx.doi.org/10.3390/ecu2021-09268.

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Garcia-Bellido, Juan. "Primordial Black Holes." In 2nd World Summit: Exploring the Dark Side of the Universe. Trieste, Italy: Sissa Medialab, 2018. http://dx.doi.org/10.22323/1.335.0042.

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Dolgov, Alexander. "Massive Primordial Black Holes." In Multifrequency Behaviour of High Energy Cosmic Sources - XIII. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.362.0013.

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Arbey, Alexandre, Jeremy Auffinger, and Joseph Silk. "Primordial Kerr Black Holes." In 40th International Conference on High Energy physics. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.390.0585.

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Harada, Tomohiro. "Growth of primordial black holes." In Proceedings of the VII Asia-Pacific International Conference. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812772923_0030.

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Musco, Ilia. "Primordial black hole formation." In Black Holes in General Relativity and String Theory. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.075.0028.

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Guariento, Daniel, and Jorge E. Horvath. "Accretion mechanisms onto primordial black holes." In 5th International School on Field Theory and Gravitation. Trieste, Italy: Sissa Medialab, 2009. http://dx.doi.org/10.22323/1.081.0059.

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LIDDLE, ANDREW R., and ANNE M. GREEN. "PRIMORDIAL BLACK HOLES AND EARLY COSMOLOGY." In Proceedings of the First International Workshop on Particle Physics and the Early Universe. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789814447263_0072.

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Majumdar, A. S., Sandip K. Chakrabarti, and Archan S. Majumdar. "Primordial black holes as dark matter." In OBSERVATIONAL EVIDENCE FOR BLACK HOLES IN THE UNIVERSE: Proceedings of the 2nd Kolkata Conference on Observational Evidence for Black Holes in the Universe held in Kolkata India, 10–15 February 2008 and the Satellite Meeting on Black Holes, Neutron Stars, and Gamma-Ray Bursts held 16–17 February 2008. AIP, 2008. http://dx.doi.org/10.1063/1.3009471.

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Reports on the topic "Inflation,Primordial Black Holes"

1

Thompson, K. Formation and Evolution of Primordial Black Holes After Hybrid Inflation. Office of Scientific and Technical Information (OSTI), March 2005. http://dx.doi.org/10.2172/839930.

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2

Black, William Kevin. Primordial Origins of Supermassive Black Holes. Office of Scientific and Technical Information (OSTI), July 2018. http://dx.doi.org/10.2172/1460661.

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Perez-Gonzalez, Yuber F., and Cecilia Lunardini. Dirac and Majorana Neutrino Signatures of Primordial Black Holes. Office of Scientific and Technical Information (OSTI), October 2019. http://dx.doi.org/10.2172/1597056.

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4

Frank Krennrich. A Search for Microsecond Gamma Ray Bursts From Primordial Black Holes. Office of Scientific and Technical Information (OSTI), August 2004. http://dx.doi.org/10.2172/827852.

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5

Wells, James D. Illuminating dark matter and primordial black holes with an interstellar antiproton spectrometer. Office of Scientific and Technical Information (OSTI), November 1998. http://dx.doi.org/10.2172/9903.

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