Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime
In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static sph...
Saved in:
Published in | Astrophysics and space science Vol. 370; no. 5; p. 46 |
---|---|
Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Dordrecht
Springer Netherlands
01.05.2025
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Abstract | In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static spherically symmetric metric. Moreover, external Schwarzschild geometry is taken into account to correlate our internal stellar structure and determine the values of the constants used in the Finch-Skea spacetime solution. Finally, in this paper, multiple aspects are discussed, such as the radius, compactness, stresses, stability, density profile, and masses under the variable cosmological constant model in
f
(
R
,
T
)
gravity for various stars. |
---|---|
AbstractList | In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static spherically symmetric metric. Moreover, external Schwarzschild geometry is taken into account to correlate our internal stellar structure and determine the values of the constants used in the Finch-Skea spacetime solution. Finally, in this paper, multiple aspects are discussed, such as the radius, compactness, stresses, stability, density profile, and masses under the variable cosmological constant model in f(R,T) gravity for various stars. In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and validates the required energy conditions (Ecs), and TOV equations. First, the Finch-Skea spacetime solution is taken into account as a static spherically symmetric metric. Moreover, external Schwarzschild geometry is taken into account to correlate our internal stellar structure and determine the values of the constants used in the Finch-Skea spacetime solution. Finally, in this paper, multiple aspects are discussed, such as the radius, compactness, stresses, stability, density profile, and masses under the variable cosmological constant model in f ( R , T ) gravity for various stars. |
ArticleNumber | 46 |
Author | Maha Sher, Falak Khan, Fawad Nawaz, Salma Ilyas, M. |
Author_xml | – sequence: 1 givenname: M. surname: Ilyas fullname: Ilyas, M. email: ilyas_mia@yahoo.com organization: Institute of Physics, Gomal University – sequence: 2 surname: Maha fullname: Maha organization: University of Management and Technology – sequence: 3 givenname: Salma surname: Nawaz fullname: Nawaz, Salma organization: Institute of Physics, Gomal University – sequence: 4 givenname: Falak surname: Sher fullname: Sher, Falak organization: Department of Materials Science and Engineering, University of Illinois Urbana-Champaign – sequence: 5 givenname: Fawad surname: Khan fullname: Khan, Fawad organization: Institute of Physics, Gomal University |
BookMark | eNp9kE1LAzEQhoMoWD_-gKeA5-hsNrtpjiJ-geBBhd7CNJ3UrbvZmqSC_97UCt48DcM87zvwHLH9MAZi7KyCiwpAX6YKGjACZCNAqboR7R6bVI2Wwqh2ts8mAKBEq2B2yI5SWpXVtEZPmHsY1ugyHz1H_omxw3lP3I1pGPtx2TnsyxJSxlCYwFOmvsfIB8yZ4vbku-UmYu4KxLvAb7vg3sTzOyFPpZhyN9AJO_DYJzr9ncfs9fbm5fpePD7dPVxfPQontcyiRvKq1mbqanQaptS0XjdSLxQhLFBBPQeC-VRXBueyVdr7yreklTG0cBLrY3a-613H8WNDKdvVuImhvLS1BAVGy2lVKLmjXBxTiuTtOnYDxi9bgd3KtDuZtsi0PzJtW0L1LpQKHJYU_6r_SX0DHl96og |
Cites_doi | 10.1088/0004-637X/693/2/1775 10.1038/nature09466 10.1103/PhysRevD.110.023013 10.1140/epjc/s10052-025-14000-8 10.1002/prop.201800092 10.1088/0264-9381/6/4/007 10.1140/epjc/s10052-021-09062-3 10.1088/1475-7516/2022/06/004 10.3847/1538-4357/ad5cf1 10.1016/j.physletb.2014.01.066 10.1016/0375-9601(92)90036-L 10.1140/epjc/s10052-022-11139-6 10.1016/j.rinp.2021.104674 10.1142/S0218271817500146 10.1142/S0219887819501494 10.1103/PhysRevD.78.024015 10.1016/j.cjph.2022.12.013 10.1140/epjc/s10052-022-10483-x 10.1103/PhysRevLett.92.241302 10.1103/PhysRevD.97.064030 10.12942/lrr-2008-9 10.1103/PhysRevD.84.024020 10.1007/s10509-017-3215-8 10.3847/1538-4365/ad0154 10.1103/PhysRevD.103.044002 10.1007/s10714-022-02927-2 10.1002/prop.202400092 10.1140/epjc/s10052-018-6232-z 10.1093/mnras/stad3562 10.1093/mnras/stt401 10.1140/epjp/s13360-024-05778-9 10.1142/S0218271800000542 10.1016/j.cjph.2024.02.022 10.1093/mnras/stac3611 10.1088/1475-7516/2011/09/018 10.1093/mnras/stad2861 10.1103/PhysRev.116.1027 10.1103/PhysRevD.94.103513 10.1103/PhysRevD.84.104035 10.1088/0004-637X/719/2/1807 10.1016/j.dark.2020.100753 10.1103/PhysRevD.97.104062 10.1103/PhysRevD.91.124019 10.1088/0004-637X/712/2/964 10.1088/1361-6382/ab75ae 10.3847/1538-4357/ac4255 |
ContentType | Journal Article |
Copyright | The Author(s), under exclusive licence to Springer Nature B.V. 2025 Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. Copyright Springer Nature B.V. May 2025 |
Copyright_xml | – notice: The Author(s), under exclusive licence to Springer Nature B.V. 2025 Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law. – notice: Copyright Springer Nature B.V. May 2025 |
DBID | AAYXX CITATION 7TG 8FD H8D KL. L7M |
DOI | 10.1007/s10509-025-04435-6 |
DatabaseName | CrossRef Meteorological & Geoastrophysical Abstracts Technology Research Database Aerospace Database Meteorological & Geoastrophysical Abstracts - Academic Advanced Technologies Database with Aerospace |
DatabaseTitle | CrossRef Aerospace Database Meteorological & Geoastrophysical Abstracts Technology Research Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts - Academic |
DatabaseTitleList | Aerospace Database |
DeliveryMethod | fulltext_linktorsrc |
Discipline | Astronomy & Astrophysics Physics |
EISSN | 1572-946X |
ExternalDocumentID | 10_1007_s10509_025_04435_6 |
GroupedDBID | -Y2 -~C -~X .86 .VR 06D 0R~ 0VY 1N0 1SB 2.D 203 23N 28- 29~ 2J2 2JN 2JY 2KG 2KM 2LR 2P1 2VQ 2WC 2~H 30V 4.4 406 408 409 40D 40E 5GY 5QI 5VS 67Z 6J9 6NX 6TJ 88I 8FE 8FG 8FH 8TC 8UJ 95- 95. 95~ 96X AAAVM AABHQ AACDK AAHNG AAIAL AAJBT AAJKR AANZL AAPKM AARHV AARTL AASML AATNV AATVU AAUYE AAWCG AAYIU AAYQN AAYTO AAYZH ABAKF ABBBX ABBRH ABBXA ABDBE ABDBF ABDZT ABECU ABFTV ABHFT ABHLI ABHQN ABJNI ABJOX ABKCH ABKTR ABMNI ABMQK ABNWP ABQBU ABQSL ABSXP ABTEG ABTHY ABTKH ABTMW ABULA ABUWG ABWNU ABXPI ACAOD ACBXY ACDTI ACGFS ACGOD ACHSB ACHXU ACKNC ACMDZ ACMFV ACMLO ACNCT ACOKC ACOMO ACPIV ACREN ACSNA ACUHS ACZOJ ADHHG ADHIR ADHKG ADIMF ADKNI ADKPE ADMLS ADRFC ADTPH ADURQ ADYFF ADYOE ADZKW AEBTG AEFIE AEFQL AEGAL AEGNC AEJHL AEJRE AEKMD AEMSY AENEX AEOHA AEPYU AESKC AETLH AEUYN AEVLU AEXYK AFBBN AFDZB AFEXP AFFNX AFGCZ AFKRA AFLOW AFOHR AFQWF AFWTZ AFYQB AFZKB AGAYW AGDGC AGGDS AGJBK AGMZJ AGQEE AGQMX AGQPQ AGRTI AGWIL AGWZB AGYKE AHAVH AHBYD AHKAY AHPBZ AHSBF AHYZX AIAKS AIGIU AIIXL AILAN AITGF AJBLW AJRNO AJZVZ ALMA_UNASSIGNED_HOLDINGS ALWAN AMKLP AMTXH AMXSW AMYLF AMYQR AOCGG ARAPS ARMRJ ASPBG ATHPR AVWKF AXYYD AYFIA AYJHY AZFZN AZQEC B-. B0M BA0 BBWZM BDATZ BENPR BGLVJ BGNMA BPHCQ BSONS CAG CCPQU COF CS3 CSCUP D1K DDRTE DL5 DNIVK DPUIP DWQXO E3Z EAD EAP EBLON EBS EIOEI EJD EMK EPL ESBYG ESX F5P FEDTE FERAY FFXSO FIGPU FINBP FNLPD FRRFC FSGXE FWDCC GGCAI GGRSB GJIRD GNUQQ GNWQR GPTSA GQ7 GQ8 GXS H13 HCIFZ HF~ HG5 HG6 HMJXF HQYDN HRMNR HVGLF HZ~ I-F I09 IHE IJ- IKXTQ ITM IWAJR IXC IZIGR IZQ I~X I~Z J-C J0Z JBSCW JCJTX JZLTJ K6- KDC KOV KOW KZ1 LAK LK5 LLZTM M2P M4Y M7R MA- N2Q NB0 NDZJH NPVJJ NQJWS NU0 O9- O93 O9G O9I O9J OAM OHT OK1 OVD P19 P62 P9T PF0 PHGZM PHGZT PQQKQ PROAC PT4 PT5 Q2X QOK QOS R4E R89 R9I RHV RNI RNS ROL RPX RSV RZC RZE RZK S16 S1Z S26 S27 S28 S3B SAP SCLPG SDH SDM SGB SHX SISQX SJYHP SNE SNPRN SNX SOHCF SOJ SPH SPISZ SRMVM SSLCW STPWE SZN T13 T16 T9H TEORI TSG TSK TSV TUC TUS U2A UG4 UOJIU UTJUX UZXMN VC2 VFIZW VOH W23 W48 WH7 WK8 XJT YLTOR Z45 ZMTXR ZY4 ~02 ~8M ~A9 ~EX AAYXX ABFSG ACSTC AEZWR AFHIU AHWEU AIXLP CITATION 7TG 8FD ABRTQ H8D KL. L7M |
ID | FETCH-LOGICAL-c272t-3aef43798c3ac708e56f7527d4ea0da403b0e0b8719ab2647ff1f6e7499edc2a3 |
IEDL.DBID | U2A |
ISSN | 0004-640X |
IngestDate | Fri Jul 25 09:33:27 EDT 2025 Thu Jul 03 08:19:18 EDT 2025 Fri May 16 02:04:47 EDT 2025 |
IsPeerReviewed | true |
IsScholarly | true |
Issue | 5 |
Keywords | Alternate to G.R Compact stars Modified theory of gravity Variable cosmological constant |
Language | English |
LinkModel | DirectLink |
MergedId | FETCHMERGED-LOGICAL-c272t-3aef43798c3ac708e56f7527d4ea0da403b0e0b8719ab2647ff1f6e7499edc2a3 |
Notes | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
PQID | 3204097281 |
PQPubID | 105598 |
ParticipantIDs | proquest_journals_3204097281 crossref_primary_10_1007_s10509_025_04435_6 springer_journals_10_1007_s10509_025_04435_6 |
PublicationCentury | 2000 |
PublicationDate | 20250500 2025-05-00 20250501 |
PublicationDateYYYYMMDD | 2025-05-01 |
PublicationDate_xml | – month: 5 year: 2025 text: 20250500 |
PublicationDecade | 2020 |
PublicationPlace | Dordrecht |
PublicationPlace_xml | – name: Dordrecht |
PublicationSubtitle | An International Journal of Astronomy, Astrophysics and Space Science |
PublicationTitle | Astrophysics and space science |
PublicationTitleAbbrev | Astrophys Space Sci |
PublicationYear | 2025 |
Publisher | Springer Netherlands Springer Nature B.V |
Publisher_xml | – name: Springer Netherlands – name: Springer Nature B.V |
References | 4435_CR30 G. Dvali (4435_CR12) 2019; 67 G. Mustafa (4435_CR41) 2024; 88 S.D. Maharaj (4435_CR29) 2017; 26 A. Ditta (4435_CR11) 2024; 139 E. Bertschinger (4435_CR3) 2008; 78 T. Güver (4435_CR18) 2010; 719 S. Dey (4435_CR10) 2020; 37 H.A. Buchdahl (4435_CR4) 1959; 116 B. Das (4435_CR7) 2022; 82 M. Ilyas (4435_CR25) 2025; 85 M. Ilyas (4435_CR23) 2019; 16 T. Harko (4435_CR19) 2011; 84 M.F. Barbat (4435_CR2) 2024; 110 S.K. Maurya (4435_CR33) 2021; 31 R.V. Maluf (4435_CR31) 2021; 103 A. Errehymy (4435_CR13) 2021; 81 S.K. Maurya (4435_CR37) 2023; 519 Y. Wang (4435_CR51) 2004; 92 T. Güver (4435_CR17) 2010; 712 B. Dayanandan (4435_CR8) 2023; 82 S.K. Maurya (4435_CR35) 2022; 925 P. Pani (4435_CR43) 2011; 84 P.B. Demorest (4435_CR9) 2010; 467 S.K. Maurya (4435_CR39) 2024; 527 F. Özel (4435_CR42) 2009; 693 M. Ilyas (4435_CR24) 2017; 362 S. Capozziello (4435_CR6) 2015; 91 S.K. Maurya (4435_CR38) 2024; 972 4435_CR16 S.V. Lohakare (4435_CR28) 2023; 526 4435_CR22 S. Pradhan (4435_CR45) 2024; 72 Z. Stuchlík (4435_CR50) 2016; 94 S.K. Maurya (4435_CR32) 2021; 29 L. Herrera (4435_CR20) 1992; 165 N.K. Largani (4435_CR27) 2019 M. Ballardini (4435_CR1) 2022; 2022 S. Capozziello (4435_CR5) 2014; 730 K. Jusufi (4435_CR26) 2018; 97 S. Shankaranarayanan (4435_CR48) 2022; 54 M. Ilyas (4435_CR21) 2018; 78 T. Gangopadhyay (4435_CR15) 2013; 431 S.K. Maurya (4435_CR36) 2023; 269 Z. Stuchlík (4435_CR49) 2011; 2011 N.E. Mavromatos (4435_CR40) 2016 S.K. Maurya (4435_CR34) 2022; 82 V. Perlick (4435_CR44) 2018; 97 V. Sahni (4435_CR47) 2000; 9 M.R. Finch (4435_CR14) 1989; 6 D. Psaltis (4435_CR46) 2008; 11 |
References_xml | – volume: 693 start-page: 1775 issue: 2 year: 2009 ident: 4435_CR42 publication-title: Astrophys. J. doi: 10.1088/0004-637X/693/2/1775 – volume: 467 start-page: 1081 issue: 7319 year: 2010 ident: 4435_CR9 publication-title: Nature (London) doi: 10.1038/nature09466 – volume: 110 issue: 2 year: 2024 ident: 4435_CR2 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.110.023013 – volume: 85 start-page: 253 issue: 3 year: 2025 ident: 4435_CR25 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-025-14000-8 – volume: 67 issue: 1–2 year: 2019 ident: 4435_CR12 publication-title: Fortschr. Phys. doi: 10.1002/prop.201800092 – volume: 6 start-page: 467 issue: 4 year: 1989 ident: 4435_CR14 publication-title: Class. Quantum Gravity doi: 10.1088/0264-9381/6/4/007 – volume: 81 start-page: 1 issue: 3 year: 2021 ident: 4435_CR13 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-021-09062-3 – volume: 2022 issue: 06 year: 2022 ident: 4435_CR1 publication-title: J. Cosmol. Astropart. Phys. doi: 10.1088/1475-7516/2022/06/004 – volume: 972 start-page: 175 issue: 2 year: 2024 ident: 4435_CR38 publication-title: Astrophys. J. doi: 10.3847/1538-4357/ad5cf1 – volume: 730 start-page: 280 year: 2014 ident: 4435_CR5 publication-title: Phys. Lett. B doi: 10.1016/j.physletb.2014.01.066 – volume: 165 start-page: 206 issue: 3 year: 1992 ident: 4435_CR20 publication-title: Phys. Lett. A doi: 10.1016/0375-9601(92)90036-L – volume: 82 start-page: 1173 issue: 12 year: 2022 ident: 4435_CR34 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-022-11139-6 – volume: 29 year: 2021 ident: 4435_CR32 publication-title: Results Phys. doi: 10.1016/j.rinp.2021.104674 – ident: 4435_CR16 – volume: 26 issue: 03 year: 2017 ident: 4435_CR29 publication-title: Int. J. Mod. Phys. D doi: 10.1142/S0218271817500146 – volume: 16 issue: 10 year: 2019 ident: 4435_CR23 publication-title: Int. J. Geom. Methods Mod. Phys. doi: 10.1142/S0219887819501494 – ident: 4435_CR22 – volume: 78 issue: 2 year: 2008 ident: 4435_CR3 publication-title: Phys. Rev. D, Part. Fields Grav. Cosmol. doi: 10.1103/PhysRevD.78.024015 – volume: 82 start-page: 155 year: 2023 ident: 4435_CR8 publication-title: Chin. J. Phys. doi: 10.1016/j.cjph.2022.12.013 – volume: 82 start-page: 519 issue: 6 year: 2022 ident: 4435_CR7 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-022-10483-x – volume: 92 issue: 24 year: 2004 ident: 4435_CR51 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.92.241302 – volume: 97 issue: 6 year: 2018 ident: 4435_CR26 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.97.064030 – volume: 11 start-page: 9 issue: 1 year: 2008 ident: 4435_CR46 publication-title: Living Rev. Relativ. doi: 10.12942/lrr-2008-9 – volume: 84 issue: 2 year: 2011 ident: 4435_CR19 publication-title: Phys. Rev. D, Part. Fields Grav. Cosmol. doi: 10.1103/PhysRevD.84.024020 – volume: 362 start-page: 237 issue: 12 year: 2017 ident: 4435_CR24 publication-title: Astrophys. Space Sci. doi: 10.1007/s10509-017-3215-8 – start-page: 09007 volume-title: EPJ Web of Conferences year: 2019 ident: 4435_CR27 – volume: 269 start-page: 35 issue: 2 year: 2023 ident: 4435_CR36 publication-title: Astrophys. J. Suppl. Ser. doi: 10.3847/1538-4365/ad0154 – volume: 103 issue: 4 year: 2021 ident: 4435_CR31 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.103.044002 – volume: 54 start-page: 44 issue: 5 year: 2022 ident: 4435_CR48 publication-title: Gen. Relativ. Gravit. doi: 10.1007/s10714-022-02927-2 – volume: 72 issue: 9–10 year: 2024 ident: 4435_CR45 publication-title: Fortschr. Phys. doi: 10.1002/prop.202400092 – volume: 78 start-page: 757 issue: 9 year: 2018 ident: 4435_CR21 publication-title: Eur. Phys. J. C doi: 10.1140/epjc/s10052-018-6232-z – volume: 527 start-page: 5192 issue: 3 year: 2024 ident: 4435_CR39 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stad3562 – volume: 431 start-page: 3216 issue: 4 year: 2013 ident: 4435_CR15 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stt401 – volume: 139 start-page: 1 issue: 11 year: 2024 ident: 4435_CR11 publication-title: Eur. Phys. J. Plus doi: 10.1140/epjp/s13360-024-05778-9 – volume: 9 start-page: 373 issue: 04 year: 2000 ident: 4435_CR47 publication-title: Int. J. Mod. Phys. D doi: 10.1142/S0218271800000542 – volume: 88 start-page: 938 year: 2024 ident: 4435_CR41 publication-title: Chin. J. Phys. doi: 10.1016/j.cjph.2024.02.022 – volume: 519 start-page: 4303 issue: 3 year: 2023 ident: 4435_CR37 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stac3611 – volume: 2011 issue: 09 year: 2011 ident: 4435_CR49 publication-title: J. Cosmol. Astropart. Phys. doi: 10.1088/1475-7516/2011/09/018 – volume: 526 start-page: 3796 issue: 3 year: 2023 ident: 4435_CR28 publication-title: Mon. Not. R. Astron. Soc. doi: 10.1093/mnras/stad2861 – volume: 116 start-page: 1027 issue: 4 year: 1959 ident: 4435_CR4 publication-title: Phys. Rev. doi: 10.1103/PhysRev.116.1027 – volume: 94 issue: 10 year: 2016 ident: 4435_CR50 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.94.103513 – volume: 84 issue: 10 year: 2011 ident: 4435_CR43 publication-title: Phys. Rev. D, Part. Fields Grav. Cosmol. doi: 10.1103/PhysRevD.84.104035 – volume: 719 start-page: 1807 issue: 2 year: 2010 ident: 4435_CR18 publication-title: Astrophys. J. doi: 10.1088/0004-637X/719/2/1807 – volume: 31 year: 2021 ident: 4435_CR33 publication-title: Phys. Dark Universe doi: 10.1016/j.dark.2020.100753 – volume: 97 issue: 10 year: 2018 ident: 4435_CR44 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.97.104062 – ident: 4435_CR30 – start-page: 02020 volume-title: EPJ Web of Conferences year: 2016 ident: 4435_CR40 – volume: 91 issue: 12 year: 2015 ident: 4435_CR6 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.91.124019 – volume: 712 start-page: 964 issue: 2 year: 2010 ident: 4435_CR17 publication-title: Astrophys. J. doi: 10.1088/0004-637X/712/2/964 – volume: 37 issue: 7 year: 2020 ident: 4435_CR10 publication-title: Class. Quantum Gravity doi: 10.1088/1361-6382/ab75ae – volume: 925 start-page: 208 issue: 2 year: 2022 ident: 4435_CR35 publication-title: Astrophys. J. doi: 10.3847/1538-4357/ac4255 |
SSID | ssj0009697 |
Score | 2.4044087 |
Snippet | In this study, a variable cosmological constant model is created for anisotropic star structures, which satisfies the remaining physical requirements, and... |
SourceID | proquest crossref springer |
SourceType | Aggregation Database Index Database Publisher |
StartPage | 46 |
SubjectTerms | Astrobiology Astronomy Astrophysics and Astroparticles Cosmological constant Cosmology Geometry Gravity Observations and Techniques Physics Physics and Astronomy Relativity Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacetime Stars & galaxies Stellar structure Theory of relativity Universe |
Title | Impact of a variable cosmological constant on stellar matter configurations in Finch-Skea spacetime |
URI | https://link.springer.com/article/10.1007/s10509-025-04435-6 https://www.proquest.com/docview/3204097281 |
Volume | 370 |
hasFullText | 1 |
inHoldings | 1 |
isFullTextHit | |
isPrint | |
link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwlV1BS8MwFH7ohuBFdCqbzpGDeNFAmjZNd9xkcyoOQQfzVNI00SHrxE7Bf2-StkxFD56akpDDy8vL95J8XwCOu1YjJdUmLRFeiAMuTRz0eIpT4YcyYIJ3heUO34zD0SS4mrJpSQrLq9vu1ZGki9RfyG7MbuRThklgFnkcrkOd2dzdePGE9lZSu8WTKhat4DAg05Iq83sf35ejFcb8cSzqVpvhNmyVMBH1inHdgTWVNaDZy-3G9WL-gU6QKxf7EnkDNm6L0i7IS8d7RAuNBHo3mbDlRiG5yOdVmDM_DhOaNhnKLYtEvKK509m0VXr2-Fa4RY5mGRrOMvmE756VQCb4SGUfo9-DyXBwfz7C5UsKWFJOl9gXSlvhwUj6QnISKRZqzihPAyVIKgLiJ0SRxCRPXZEYiMS19nSouEmHVCqp8Pehli0y1QTkRVIYjKIVFVGgmZdoE0611JKRlHmatOC0Mmj8UghmxCtpZGv-2Jg_duaPwxa0K5vH5eTJY58Sq8JFI68FZ9U4rKr_7u3gf80PYZM6V7DXF9tQW76-qSMDMZZJB-q9Yb8_tt-Lh-tBx3nYJwsxy-Y |
linkProvider | Springer Nature |
linkToHtml | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwlV3PS8MwFH7oRPQi_mTTqTmIFw2kadN0xyGOTTcR3GC3kqaJDlkn6yb435ukLVPRg7eUhBxe0ve-l-T7HsBFy2qkpNqkJcILccCl8YMeT3Eq_FAGTPCWsNzhwUPYHQV3YzYuSWF59dq9upJ0nvoL2Y3Zg3zKMAlMkMfhOmwYMBDZh1wj2l5J7RYlVSxawWFAxiVV5vc5voejFcb8cS3qok1nF3ZKmIjaxbruwZrK9qHezu3B9Wz6gS6RaxfnEvk-bD4WrQOQPcd7RDONBHo3mbDlRiE5y6eVmzMfDhOaMRnKLYtEzNHU6WzaLj15XhbbIkeTDHUmmXzBT69KION8pLLF6A9h1Lkd3nRxWUkBS8rpAvtCaSs8GElfSE4ixULNGeVpoARJRUD8hCiSmOSpJRIDkbjWng4VN-mQSiUV_hHUslmm6oC8SAqDUbSiIgo08xJt3KmWWjKSMk-TBlxVBo3fCsGMeCWNbM0fG_PHzvxx2IBmZfO4_Hny2KfEqnDRyGvAdbUOq-6_Zzv-3_Bz2OoOB_2433u4P4Ft6raFfcrYhNpivlSnBm4skjO3uz4BBQfLyQ |
linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwlV1LS8QwEB58oHgRn-z6zEG8aDBNm6Z7XNTFN4Iu7K2kaaKLbLtsu4L_3iTdUhU9eEtJyGEynfkmyfcF4KhjNVJSbcoS4YU44NLEQY-nOBV-KAMmeEdY7vD9Q3jVD24GbPCFxe9uu9dHkhWnwao0ZeXZONVnX4hvzG7qU4ZJYBI-Dudh0YRjz_p1n3Yb2d3qeRWLXHAYkMGMNvP7HN9TU4M3fxyRuszTW4PVGWRE3WqN12FOZRvQ6hZ2EzsffaBj5NrVHkWxAUuPVWsT5LXjQKJcI4HeTVVseVJI5sWoDnnmw-FDMyZDhWWUiAkaOc1N26WHL9PKRQo0zFBvmMlX_PSmBDKBSCr7MP0W9HuXz-dXePaqApaU0xL7QmkrQhhJX0hOIsVCzRnlaaAESUVA_IQokphCqiMSA5e41p4OFTelkUolFf42LGR5plqAvEgKg1e0oiIKNPMSbUKrlloykjJPkzac1AaNx5V4RtzIJFvzx8b8sTN_HLZhr7Z5PPuRitinxCpy0chrw2m9Dk3337Pt_G_4ISw_XvTiu-uH211Yoc4r7K3GPVgoJ1O1b5BHmRw45_oE833QBQ |
openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Impact+of+a+variable+cosmological+constant+on+stellar+matter+configurations+in+Finch-Skea+spacetime&rft.jtitle=Astrophysics+and+space+science&rft.au=Ilyas%2C+M.&rft.au=Maha&rft.au=Nawaz%2C+Salma&rft.au=Sher%2C+Falak&rft.date=2025-05-01&rft.issn=0004-640X&rft.eissn=1572-946X&rft.volume=370&rft.issue=5&rft_id=info:doi/10.1007%2Fs10509-025-04435-6&rft.externalDBID=n%2Fa&rft.externalDocID=10_1007_s10509_025_04435_6 |
thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-640X&client=summon |
thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-640X&client=summon |
thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-640X&client=summon |