Md Khurshid Alam

S. Surendra Singh

L. Anjana Devi

Erratum to “Interaction of Anisotropic Dark Energy with Generalized Hybrid Expansion Law”

Linyu Chen

Hu Deng

Zhixiang Wu

Zhonggang Xiong

Jin Guo

Quancheng Liu

Akwasi Danso Samuel

Liping Shang

Erratum to “Role of Focusing Distance in Picosecond Laser-Induced Cu Plasma Spectra”

Abel Mukubwa

Erratum to “Electron Number Density and Coherence Length of Boson-Fermion Pair in HTSC”

Carlos Frajuca

Fabio da Silva Bortoli

Nadja Simao Magalhaes

Erratum to “The Analysis of a Proposed Experiment to Measure the Speed of Gravity in Short Distances”

Gianni Albertini

Fabio Cardone

Stefano Bellucci

Erratum to “The Asymmetry of the Cosmic Microwave Background Radiation as Signature of Local Lorentz Invariance Violation”

D. M. Mostafa

Erratum to “Linear Stability of Magneto Viscoelastic Walter’s <italic>B</italic><svg  xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"   style="vertical-align:-0.04981995pt" height="7.86364pt" version="1.1" viewBox="-0.0498162 -7.81382 4.53621 7.86364" width="4.53621pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><path id="g113-31" d="M295 534L291 558C277 573 202 603 180 597L75 72L120 51L295 534Z" /></g></svg>Type with Heat and Mass Transfer”

In this work, we study thermodynamics of generalized Ayon-Beato and Garcia (ABG) black hole metric which contains three parameters named as mass <span class="nowrap"><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-0.2063904pt" id="M1" height="6.1673pt" version="1.1" viewBox="-0.0498162 -5.96091 10.3951 6.1673" width="10.3951pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><path id="g113-110" d="M766 88L752 113C719 83 690 64 681 64C674 64 672 74 679 103L724 292C758 436 724 448 701 448C680 448 666 442 639 429C594 407 514 350 441 252H439L447 289C476 423 450 448 419 448C398 448 379 441 355 427C307 400 234 344 162 249H160L180 324C203 409 197 448 170 448C144 448 82 413 23 349L35 321C57 343 96 374 108 374C115 374 117 371 111 341C87 227 57 112 24 -6L32 -12C53 -4 81 4 108 6C119 68 134 128 149 171C177 229 309 383 364 383C387 383 388 355 373 282C354 190 330 92 303 -6L309 -12C332 -4 356 3 386 6C396 63 411 122 424 171C458 236 590 383 642 383C658 383 664 369 652 315L603 91C587 20 593 -12 619 -12C642 -12 708 23 766 88Z"/></g></svg>,</span> magnetic charge <span class="nowrap"><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-3.42943pt" id="M2" height="9.39034pt" version="1.1" viewBox="-0.0498162 -5.96091 6.50656 9.39034" width="6.50656pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><path id="g113-114" d="M474 429L457 433C435 440 389 448 367 448C348 448 323 446 309 443C266 434 195 406 148 366C78 307 23 210 23 101C23 35 55 -12 92 -12C118 -12 146 1 196 35C247 70 311 130 346 173H348L281 -148C268 -211 256 -221 208 -229L191 -232L187 -257L433 -245L437 -219L411 -216C357 -210 350 -205 362 -140L427 207C447 315 461 381 474 429ZM387 387C379 337 363 262 355 236C318 180 201 57 142 57C126 57 112 81 112 128C112 205 150 321 220 376C244 395 280 403 312 403C345 403 370 396 387 387Z"/></g></svg>,</span> and dimensionless coupling constant of nonlinear electrodynamics interacting field <span class="nowrap"><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-3.42943pt" id="M3" height="9.39034pt" version="1.1" viewBox="-0.0498162 -5.96091 6.63704 9.39034" width="6.63704pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><path id="g113-225" d="M478 372C478 418 458 448 431 448C409 448 389 431 389 410C389 404 391 400 394 395C398 388 406 371 406 348C406 253 308 122 251 51H249C254 122 249 257 231 336C212 421 189 448 159 448C126 448 75 412 23 327L48 306C83 354 103 371 115 371C125 371 134 360 144 334C185 224 192 64 183 -19C146 -100 116 -202 110 -244L125 -261C154 -259 208 -234 222 -220C222 -194 225 -84 235 -23C247 -3 273 36 308 79C379 165 478 288 478 372Z"/></g></svg>.</span> We showed that central regions of this black hole behaves as dS (AdS) vacuum space by setting <span class="inline_break"><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" width="17.646pt" style="vertical-align:-3.42947pt" id="M4" height="12.7178pt" version="1.1" viewBox="-0.0498162 -9.28833 17.646 12.7178"><g transform="matrix(.013,0,0,-0.013,0,0)"><use xlink:href="#g113-114"/></g><g transform="matrix(.013,0,0,-0.013,10.015,0)"><path id="g117-91" d="M512 -3V55L134 254V256L512 456V514L75 281V230L512 -3Z"/></g></svg><span class="irelop"></span><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" width="38.641pt" style="vertical-align:-3.42947pt" height="12.7178pt" version="1.1" viewBox="21.2281838 -9.28833 38.641 12.7178"><g transform="matrix(.013,0,0,-0.013,21.278,0)"><path id="g113-51" d="M412 140C382 77 369 73 315 73H129L270 222C362 320 402 379 402 466C402 571 322 635 234 635C177 635 130 609 99 576L42 495L64 475C90 514 133 568 201 568C274 568 318 519 318 435C318 349 255 267 193 193C144 135 87 78 32 23V0H405C417 45 427 89 440 131L412 140Z"/></g><g transform="matrix(.013,0,0,-0.013,27.518,0)"><use xlink:href="#g113-110"/></g><g transform="matrix(.013,0,0,-0.013,37.775,0)"><path id="g113-41" d="M300 -147C201 -63 143 98 143 270S200 602 300 686L282 710C136 610 70 450 70 271V270C70 89 136 -72 282 -170L300 -147Z"/></g><g transform="matrix(.013,0,0,-0.013,42.273,0)"><use xlink:href="#g113-114"/></g><g transform="matrix(.013,0,0,-0.013,52.288,0)"><path id="g117-92" d="M512 230V281L75 514V456L453 256V254L75 55V-3L512 230Z"/></g></svg><span class="irelop"></span><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" width="21.357pt" style="vertical-align:-3.42947pt" height="12.7178pt" version="1.1" viewBox="63.5011838 -9.28833 21.357 12.7178"><g transform="matrix(.013,0,0,-0.013,63.551,0)"><use xlink:href="#g113-51"/></g><g transform="matrix(.013,0,0,-0.013,69.791,0)"><use xlink:href="#g113-110"/></g><g transform="matrix(.013,0,0,-0.013,80.048,0)"><path id="g113-42" d="M275 270C275 450 212 609 64 710L45 686C145 604 203 442 203 270S147 -63 45 -147L64 -170C213 -68 275 89 275 270Z"/></g></svg></span> and in the case <span class="inline_break"><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" width="17.646pt" style="vertical-align:-3.42938pt" id="M5" height="11.7782pt" version="1.1" viewBox="-0.0498162 -8.34882 17.646 11.7782"><g transform="matrix(.013,0,0,-0.013,0,0)"><use xlink:href="#g113-114"/></g><g transform="matrix(.013,0,0,-0.013,10.015,0)"><path id="g117-34" d="M535 323V373H52V323H535ZM535 138V188H52V138H535Z"/></g></svg><span class="irelop"></span><svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" width="16.711pt" style="vertical-align:-3.42938pt" height="11.7782pt" version="1.1" viewBox="21.2281838 -8.34882 16.711 11.7782"><g transform="matrix(.013,0,0,-0.013,21.278,0)"><use xlink:href="#g113-51"/></g><g transform="matrix(.013,0,0,-0.013,27.518,0)"><use xlink:href="#g113-110"/></g></svg></span> reaches to a flat Minkowski space. In the large distances, this black hole behaves as a Reissner-Nordstrom BH. However, an important role of the charge<svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-3.42943pt" id="M6" height="9.39034pt" version="1.1" viewBox="-0.0498162 -5.96091 6.50656 9.39034" width="6.50656pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><use xlink:href="#g113-114"/></g></svg> appeared in the production of a formal variable cosmological parameter which will support pressure coordinate in the thermodynamic perspective of this black hole in our setup. We should point that this formal variable cosmological parameter is different with cosmological constant which comes from AdS/CFT correspondence, and it is effective at large distances as AdS space pressure. In our setup, the assumed pressure originated from the internal material of the black hole say <svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-3.42943pt" id="M7" height="9.39034pt" version="1.1" viewBox="-0.0498162 -5.96091 6.50656 9.39034" width="6.50656pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><use xlink:href="#g113-114"/></g></svg> and <svg xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg" style="vertical-align:-0.2063904pt" id="M8" height="6.1673pt" version="1.1" viewBox="-0.0498162 -5.96091 10.3951 6.1673" width="10.3951pt"><g transform="matrix(.013,0,0,-0.013,0,0)"><use xlink:href="#g113-110"/></g></svg> here. By calculating the Hawking temperature of this black hole, we obtain equation of state. Then, we plotted isothermal P-V curves and heat capacity at constant pressure. They show that the system participates in the small to large phase transition of the black hole or the Hawking-Page phase transition which is similar to the van der Waals phase transition in the ordinary thermodynamics systems. In fact in the Hawking-Page phase transition disequilibrium, evaporating generalized ABG black hole reaches to a vacuum AdS space finally.

Elham Ghasemi

Hossein Ghaffarnejad

Thermodynamic Phase Transition of Generalized Ayon-Beato Garcia Black Holes

About this journal

<p><em>Advances in High Energy Physics</em> publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter.</p>


Journal profile

Meet the editorial board

<p>Chief Editor, Professor Seidel, is a professor in the Department of Physics and Astronomy at the University of New Mexico. She is a collaborator on the ATLAS experiment at the Large Hadron Collider, researching high-energy collider physics.</p>


Editor spotlight

Submit to Special Issue

We currently have a number of Special Issues open for submission. Special Issues highlight emerging areas of research within a field, or provide a venue for a deeper investigation into an existing research area.

Special Issues

Author guidelines

Editorial board

Databases and indexing

Advances in High Energy Physics - Table of contents 2023

Advances in High Energy Physics | Hindawi

title

Advances in High Energy Physics publishes the results of theoretical and experimental research on the nature of, and interaction between, energy and matter.

Advances in High Energy Physics